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ASTRO: Arp 295 a Zwicky connected system
Arp 295 is another Zwicky connected pair of galaxies. The southern one
is MCG -04-60-021 which is classed as Sc? pec and is a possibly LINER galaxy. The northern component is MCG-01-60-022 and classed as Sb pec. The really weird thing about it I don't see mentioned anyplace. That is its western half is brighter than the eastern. It seems to have a very sudden change of intensity running nearly vertically but slightly northeast to southwest right through the core. Very weird. The pair is located in the northeastern corner of Aquarius just across the border from Pisces. The distance to this pair is a bit difficult to pin down. Since they are obviously connected they are at the same distance yet their red shifts denoting relative velocity as well as distance are quite different. By redshift the southern galaxy is 284 million light years away while the northern is 301. Most of the other "major" galaxies in the image have red shifts of about 280 to 295 million light years so it is likely this is about the correct distance to these two as well. IC 1505, the large elliptical like galaxy to the northwest has a red shift distance of 281 million light years. About all I find on it is are several comments that it is NOT Arp 295 as some authorities apparently claim. 2MASX J23420451-0334508 the spiral above the northern component of Arp 295 is at 296 million light years. There are three small galaxies directly west of the southern component. The faintest and furthest west is GALEX 2502913013803127866 an X ray galaxy at 291 million light years. The middle one is APMUKS(BJ) B233906.66-035605.1 at 284 million light years and the eastern galaxy is MRK 0933, a compact galaxy at 285 million light years. The face on spiral at the top of the image is APMUKS(BJ) B233913.30-034624.3 at 298 million light years. The apparent edge on blue galaxy to its east (left) is APMUKS(BJ) B233934.16-034639.4 at 296 million light years. While the elliptical southwest of the face on spiral and northwest of IC 1505 is 2MASX J23412885-0331266 at 288 million light years. The face on spiral nearly due west (right) of the lower component of Arp 295 is 2MASX J23411291-0337538 at 295 million light years. Not all galaxies in the image are members of the group. At the top of the image directly above the near edge on blue galaxy APMUKS(BJ) B233934.16-034639.4 is 2MASX J23420657-0328278 at 1.5 billion light years. To its east (left) just above my image but coming into it as a fuzzy halo is 2MASX J23422688-0327555 at 620 million light years. There are 4 asteroids in the image. The faintest is closest to Arp 295 about half way between the northern component and IC 1505. It is (186080) 2001 SO230 at magnitude 19.2. Above it and slightly left is the brightest asteroid, 220052) 2002 RY101 at 18.0. Above IC 1505 and level with the face on spiral near the top of the image is 2002 TD17 at magnitude 18.7. These last two are moving only in right ascension which is rare. The final asteroid slightly below center near the right edge. It is (136974) 1998 RO50 at magnitude 18.2. The reason the asteroids are sending a sloppy "A" in International Morris Code is that I took 6 frames but the second was lost to clouds. That created a gap in the trail but shows they were in retrograde motion moving west in the sky at the time I took the image. The "dot" is fainter than the rest of the trail as that image was partly lost to clouds as well. One advantage to not needing to guide is that you don't loose the target when clouds hit. It just picks up where you left off without me doing anything. In fact I was probably sound asleep when it happened. The night was very hazy with lots of gunk over the lake that I was imaging through. This created nasty halos about many stars. Seeing this when I started I set the system for 6 rather than my normal 4 Lumanosity and 4 rather than my normal 2 for color data but clouds wiped out one L and the last two red and first two green images. I really need to redo this one this fall under better skies. This field is out of the Sloan survey area but I did find a shot of this group taken by the one meter scope at the Naval Observatory in Flagstaff. Note they put the distance at 250 million light years. I don't know how this was determined. http://apod.nasa.gov/apod/ap051008.html Arp's image: http://nedwww.ipac.caltech.edu/level...ig_arp295.jpeg 14" LX200R @ f/10, L=5x10' RG=2x10'x3 B=4x10'x3, STL-11000XM, Paramount ME Rick -- Correct domain name is arvig and it is net not com. Prefix is correct. Third character is a zero rather than a capital "Oh". |
#2
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ASTRO: Arp 295 a Zwicky connected system
Impressive!
On Sun, 11 Jul 2010 03:36:48 -0500, Rick Johnson wrote: Arp 295 is another Zwicky connected pair of galaxies. The southern one is MCG -04-60-021 which is classed as Sc? pec and is a possibly LINER galaxy. The northern component is MCG-01-60-022 and classed as Sb pec. The really weird thing about it I don't see mentioned anyplace. That is its western half is brighter than the eastern. It seems to have a very sudden change of intensity running nearly vertically but slightly northeast to southwest right through the core. Very weird. The pair is located in the northeastern corner of Aquarius just across the border from Pisces. The distance to this pair is a bit difficult to pin down. Since they are obviously connected they are at the same distance yet their red shifts denoting relative velocity as well as distance are quite different. By redshift the southern galaxy is 284 million light years away while the northern is 301. Most of the other "major" galaxies in the image have red shifts of about 280 to 295 million light years so it is likely this is about the correct distance to these two as well. IC 1505, the large elliptical like galaxy to the northwest has a red shift distance of 281 million light years. About all I find on it is are several comments that it is NOT Arp 295 as some authorities apparently claim. 2MASX J23420451-0334508 the spiral above the northern component of Arp 295 is at 296 million light years. There are three small galaxies directly west of the southern component. The faintest and furthest west is GALEX 2502913013803127866 an X ray galaxy at 291 million light years. The middle one is APMUKS(BJ) B233906.66-035605.1 at 284 million light years and the eastern galaxy is MRK 0933, a compact galaxy at 285 million light years. The face on spiral at the top of the image is APMUKS(BJ) B233913.30-034624.3 at 298 million light years. The apparent edge on blue galaxy to its east (left) is APMUKS(BJ) B233934.16-034639.4 at 296 million light years. While the elliptical southwest of the face on spiral and northwest of IC 1505 is 2MASX J23412885-0331266 at 288 million light years. The face on spiral nearly due west (right) of the lower component of Arp 295 is 2MASX J23411291-0337538 at 295 million light years. Not all galaxies in the image are members of the group. At the top of the image directly above the near edge on blue galaxy APMUKS(BJ) B233934.16-034639.4 is 2MASX J23420657-0328278 at 1.5 billion light years. To its east (left) just above my image but coming into it as a fuzzy halo is 2MASX J23422688-0327555 at 620 million light years. There are 4 asteroids in the image. The faintest is closest to Arp 295 about half way between the northern component and IC 1505. It is (186080) 2001 SO230 at magnitude 19.2. Above it and slightly left is the brightest asteroid, 220052) 2002 RY101 at 18.0. Above IC 1505 and level with the face on spiral near the top of the image is 2002 TD17 at magnitude 18.7. These last two are moving only in right ascension which is rare. The final asteroid slightly below center near the right edge. It is (136974) 1998 RO50 at magnitude 18.2. The reason the asteroids are sending a sloppy "A" in International Morris Code is that I took 6 frames but the second was lost to clouds. That created a gap in the trail but shows they were in retrograde motion moving west in the sky at the time I took the image. The "dot" is fainter than the rest of the trail as that image was partly lost to clouds as well. One advantage to not needing to guide is that you don't loose the target when clouds hit. It just picks up where you left off without me doing anything. In fact I was probably sound asleep when it happened. The night was very hazy with lots of gunk over the lake that I was imaging through. This created nasty halos about many stars. Seeing this when I started I set the system for 6 rather than my normal 4 Lumanosity and 4 rather than my normal 2 for color data but clouds wiped out one L and the last two red and first two green images. I really need to redo this one this fall under better skies. This field is out of the Sloan survey area but I did find a shot of this group taken by the one meter scope at the Naval Observatory in Flagstaff. Note they put the distance at 250 million light years. I don't know how this was determined. http://apod.nasa.gov/apod/ap051008.html Arp's image: http://nedwww.ipac.caltech.edu/level...ig_arp295.jpeg 14" LX200R @ f/10, L=5x10' RG=2x10'x3 B=4x10'x3, STL-11000XM, Paramount ME Rick |
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ASTRO: Arp 295 a Zwicky connected system
Are you sure that isn't a frog with a sticky tongue?
that's so cool it defies words! "Rick Johnson" wrote in message . com... Arp 295 is another Zwicky connected pair of galaxies. The southern one is MCG -04-60-021 which is classed as Sc? pec and is a possibly LINER galaxy. The northern component is MCG-01-60-022 and classed as Sb pec. The really weird thing about it I don't see mentioned anyplace. That is its western half is brighter than the eastern. It seems to have a very sudden change of intensity running nearly vertically but slightly northeast to southwest right through the core. Very weird. The pair is located in the northeastern corner of Aquarius just across the border from Pisces. The distance to this pair is a bit difficult to pin down. Since they are obviously connected they are at the same distance yet their red shifts denoting relative velocity as well as distance are quite different. By redshift the southern galaxy is 284 million light years away while the northern is 301. Most of the other "major" galaxies in the image have red shifts of about 280 to 295 million light years so it is likely this is about the correct distance to these two as well. IC 1505, the large elliptical like galaxy to the northwest has a red shift distance of 281 million light years. About all I find on it is are several comments that it is NOT Arp 295 as some authorities apparently claim. 2MASX J23420451-0334508 the spiral above the northern component of Arp 295 is at 296 million light years. There are three small galaxies directly west of the southern component. The faintest and furthest west is GALEX 2502913013803127866 an X ray galaxy at 291 million light years. The middle one is APMUKS(BJ) B233906.66-035605.1 at 284 million light years and the eastern galaxy is MRK 0933, a compact galaxy at 285 million light years. The face on spiral at the top of the image is APMUKS(BJ) B233913.30-034624.3 at 298 million light years. The apparent edge on blue galaxy to its east (left) is APMUKS(BJ) B233934.16-034639.4 at 296 million light years. While the elliptical southwest of the face on spiral and northwest of IC 1505 is 2MASX J23412885-0331266 at 288 million light years. The face on spiral nearly due west (right) of the lower component of Arp 295 is 2MASX J23411291-0337538 at 295 million light years. Not all galaxies in the image are members of the group. At the top of the image directly above the near edge on blue galaxy APMUKS(BJ) B233934.16-034639.4 is 2MASX J23420657-0328278 at 1.5 billion light years. To its east (left) just above my image but coming into it as a fuzzy halo is 2MASX J23422688-0327555 at 620 million light years. There are 4 asteroids in the image. The faintest is closest to Arp 295 about half way between the northern component and IC 1505. It is (186080) 2001 SO230 at magnitude 19.2. Above it and slightly left is the brightest asteroid, 220052) 2002 RY101 at 18.0. Above IC 1505 and level with the face on spiral near the top of the image is 2002 TD17 at magnitude 18.7. These last two are moving only in right ascension which is rare. The final asteroid slightly below center near the right edge. It is (136974) 1998 RO50 at magnitude 18.2. The reason the asteroids are sending a sloppy "A" in International Morris Code is that I took 6 frames but the second was lost to clouds. That created a gap in the trail but shows they were in retrograde motion moving west in the sky at the time I took the image. The "dot" is fainter than the rest of the trail as that image was partly lost to clouds as well. One advantage to not needing to guide is that you don't loose the target when clouds hit. It just picks up where you left off without me doing anything. In fact I was probably sound asleep when it happened. The night was very hazy with lots of gunk over the lake that I was imaging through. This created nasty halos about many stars. Seeing this when I started I set the system for 6 rather than my normal 4 Lumanosity and 4 rather than my normal 2 for color data but clouds wiped out one L and the last two red and first two green images. I really need to redo this one this fall under better skies. This field is out of the Sloan survey area but I did find a shot of this group taken by the one meter scope at the Naval Observatory in Flagstaff. Note they put the distance at 250 million light years. I don't know how this was determined. http://apod.nasa.gov/apod/ap051008.html Arp's image: http://nedwww.ipac.caltech.edu/level...ig_arp295.jpeg 14" LX200R @ f/10, L=5x10' RG=2x10'x3 B=4x10'x3, STL-11000XM, Paramount ME Rick -- Correct domain name is arvig and it is net not com. Prefix is correct. Third character is a zero rather than a capital "Oh". |
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ASTRO: Arp 295 a Zwicky connected system
If that's his tongue what is it that's coming out the other end? I
don't think I want to know. Makes you wonder that if we were orbiting a sun in that tidal plume, how would that have changed our astronomical heritage? We'd see a very different sky that is for sure. Rick On 7/12/2010 9:38 AM, Richard Crisp wrote: Are you sure that isn't a frog with a sticky tongue? that's so cool it defies words! "Rick wrote in message . com... Arp 295 is another Zwicky connected pair of galaxies. The southern one is MCG -04-60-021 which is classed as Sc? pec and is a possibly LINER galaxy. The northern component is MCG-01-60-022 and classed as Sb pec. The really weird thing about it I don't see mentioned anyplace. That is its western half is brighter than the eastern. It seems to have a very sudden change of intensity running nearly vertically but slightly northeast to southwest right through the core. Very weird. The pair is located in the northeastern corner of Aquarius just across the border from Pisces. The distance to this pair is a bit difficult to pin down. Since they are obviously connected they are at the same distance yet their red shifts denoting relative velocity as well as distance are quite different. By redshift the southern galaxy is 284 million light years away while the northern is 301. Most of the other "major" galaxies in the image have red shifts of about 280 to 295 million light years so it is likely this is about the correct distance to these two as well. IC 1505, the large elliptical like galaxy to the northwest has a red shift distance of 281 million light years. About all I find on it is are several comments that it is NOT Arp 295 as some authorities apparently claim. 2MASX J23420451-0334508 the spiral above the northern component of Arp 295 is at 296 million light years. There are three small galaxies directly west of the southern component. The faintest and furthest west is GALEX 2502913013803127866 an X ray galaxy at 291 million light years. The middle one is APMUKS(BJ) B233906.66-035605.1 at 284 million light years and the eastern galaxy is MRK 0933, a compact galaxy at 285 million light years. The face on spiral at the top of the image is APMUKS(BJ) B233913.30-034624.3 at 298 million light years. The apparent edge on blue galaxy to its east (left) is APMUKS(BJ) B233934.16-034639.4 at 296 million light years. While the elliptical southwest of the face on spiral and northwest of IC 1505 is 2MASX J23412885-0331266 at 288 million light years. The face on spiral nearly due west (right) of the lower component of Arp 295 is 2MASX J23411291-0337538 at 295 million light years. Not all galaxies in the image are members of the group. At the top of the image directly above the near edge on blue galaxy APMUKS(BJ) B233934.16-034639.4 is 2MASX J23420657-0328278 at 1.5 billion light years. To its east (left) just above my image but coming into it as a fuzzy halo is 2MASX J23422688-0327555 at 620 million light years. There are 4 asteroids in the image. The faintest is closest to Arp 295 about half way between the northern component and IC 1505. It is (186080) 2001 SO230 at magnitude 19.2. Above it and slightly left is the brightest asteroid, 220052) 2002 RY101 at 18.0. Above IC 1505 and level with the face on spiral near the top of the image is 2002 TD17 at magnitude 18.7. These last two are moving only in right ascension which is rare. The final asteroid slightly below center near the right edge. It is (136974) 1998 RO50 at magnitude 18.2. The reason the asteroids are sending a sloppy "A" in International Morris Code is that I took 6 frames but the second was lost to clouds. That created a gap in the trail but shows they were in retrograde motion moving west in the sky at the time I took the image. The "dot" is fainter than the rest of the trail as that image was partly lost to clouds as well. One advantage to not needing to guide is that you don't loose the target when clouds hit. It just picks up where you left off without me doing anything. In fact I was probably sound asleep when it happened. The night was very hazy with lots of gunk over the lake that I was imaging through. This created nasty halos about many stars. Seeing this when I started I set the system for 6 rather than my normal 4 Lumanosity and 4 rather than my normal 2 for color data but clouds wiped out one L and the last two red and first two green images. I really need to redo this one this fall under better skies. This field is out of the Sloan survey area but I did find a shot of this group taken by the one meter scope at the Naval Observatory in Flagstaff. Note they put the distance at 250 million light years. I don't know how this was determined. http://apod.nasa.gov/apod/ap051008.html Arp's image: http://nedwww.ipac.caltech.edu/level...ig_arp295.jpeg 14" LX200R @ f/10, L=5x10' RG=2x10'x3 B=4x10'x3, STL-11000XM, Paramount ME Rick -- Correct domain name is arvig and it is net not com. Prefix is correct. Third character is a zero rather than a capital "Oh". -- Correct domain name is arvig and it is net not com. Prefix is correct. Third character is a zero rather than a capital "Oh". |
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ASTRO: Arp 295 a Zwicky connected system
Wow, that's what I call a tidal tail. I wonder if the straightness of the
tail is caused by our angle of view or if it is real... Stefan "Rick Johnson" schrieb im Newsbeitrag . com... Arp 295 is another Zwicky connected pair of galaxies. The southern one is MCG -04-60-021 which is classed as Sc? pec and is a possibly LINER galaxy. The northern component is MCG-01-60-022 and classed as Sb pec. The really weird thing about it I don't see mentioned anyplace. That is its western half is brighter than the eastern. It seems to have a very sudden change of intensity running nearly vertically but slightly northeast to southwest right through the core. Very weird. The pair is located in the northeastern corner of Aquarius just across the border from Pisces. The distance to this pair is a bit difficult to pin down. Since they are obviously connected they are at the same distance yet their red shifts denoting relative velocity as well as distance are quite different. By redshift the southern galaxy is 284 million light years away while the northern is 301. Most of the other "major" galaxies in the image have red shifts of about 280 to 295 million light years so it is likely this is about the correct distance to these two as well. IC 1505, the large elliptical like galaxy to the northwest has a red shift distance of 281 million light years. About all I find on it is are several comments that it is NOT Arp 295 as some authorities apparently claim. 2MASX J23420451-0334508 the spiral above the northern component of Arp 295 is at 296 million light years. There are three small galaxies directly west of the southern component. The faintest and furthest west is GALEX 2502913013803127866 an X ray galaxy at 291 million light years. The middle one is APMUKS(BJ) B233906.66-035605.1 at 284 million light years and the eastern galaxy is MRK 0933, a compact galaxy at 285 million light years. The face on spiral at the top of the image is APMUKS(BJ) B233913.30-034624.3 at 298 million light years. The apparent edge on blue galaxy to its east (left) is APMUKS(BJ) B233934.16-034639.4 at 296 million light years. While the elliptical southwest of the face on spiral and northwest of IC 1505 is 2MASX J23412885-0331266 at 288 million light years. The face on spiral nearly due west (right) of the lower component of Arp 295 is 2MASX J23411291-0337538 at 295 million light years. Not all galaxies in the image are members of the group. At the top of the image directly above the near edge on blue galaxy APMUKS(BJ) B233934.16-034639.4 is 2MASX J23420657-0328278 at 1.5 billion light years. To its east (left) just above my image but coming into it as a fuzzy halo is 2MASX J23422688-0327555 at 620 million light years. There are 4 asteroids in the image. The faintest is closest to Arp 295 about half way between the northern component and IC 1505. It is (186080) 2001 SO230 at magnitude 19.2. Above it and slightly left is the brightest asteroid, 220052) 2002 RY101 at 18.0. Above IC 1505 and level with the face on spiral near the top of the image is 2002 TD17 at magnitude 18.7. These last two are moving only in right ascension which is rare. The final asteroid slightly below center near the right edge. It is (136974) 1998 RO50 at magnitude 18.2. The reason the asteroids are sending a sloppy "A" in International Morris Code is that I took 6 frames but the second was lost to clouds. That created a gap in the trail but shows they were in retrograde motion moving west in the sky at the time I took the image. The "dot" is fainter than the rest of the trail as that image was partly lost to clouds as well. One advantage to not needing to guide is that you don't loose the target when clouds hit. It just picks up where you left off without me doing anything. In fact I was probably sound asleep when it happened. The night was very hazy with lots of gunk over the lake that I was imaging through. This created nasty halos about many stars. Seeing this when I started I set the system for 6 rather than my normal 4 Lumanosity and 4 rather than my normal 2 for color data but clouds wiped out one L and the last two red and first two green images. I really need to redo this one this fall under better skies. This field is out of the Sloan survey area but I did find a shot of this group taken by the one meter scope at the Naval Observatory in Flagstaff. Note they put the distance at 250 million light years. I don't know how this was determined. http://apod.nasa.gov/apod/ap051008.html Arp's image: http://nedwww.ipac.caltech.edu/level...ig_arp295.jpeg 14" LX200R @ f/10, L=5x10' RG=2x10'x3 B=4x10'x3, STL-11000XM, Paramount ME Rick -- Correct domain name is arvig and it is net not com. Prefix is correct. Third character is a zero rather than a capital "Oh". |
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ASTRO: Arp 295 a Zwicky connected system
Good question. I'm going with real as the chance of such an alignment
to make a curved plume so straight seems rather small. Back in the 80's I used a big computer (weaker than my laptop today) to model some galaxy collisions. I found it quite possible to get straight plumes connecting the galaxies if the speed was high enough they paths weren't altered significantly. If they would eventually merge then the plumes were less well defined and curved. Often highly curved. I should find that code and redo it as today I could include more parameters that might change the result. Rick On 7/21/2010 5:04 PM, Stefan Lilge wrote: Wow, that's what I call a tidal tail. I wonder if the straightness of the tail is caused by our angle of view or if it is real... Stefan "Rick schrieb im Newsbeitrag . com... Arp 295 is another Zwicky connected pair of galaxies. The southern one is MCG -04-60-021 which is classed as Sc? pec and is a possibly LINER galaxy. The northern component is MCG-01-60-022 and classed as Sb pec. The really weird thing about it I don't see mentioned anyplace. That is its western half is brighter than the eastern. It seems to have a very sudden change of intensity running nearly vertically but slightly northeast to southwest right through the core. Very weird. The pair is located in the northeastern corner of Aquarius just across the border from Pisces. The distance to this pair is a bit difficult to pin down. Since they are obviously connected they are at the same distance yet their red shifts denoting relative velocity as well as distance are quite different. By redshift the southern galaxy is 284 million light years away while the northern is 301. Most of the other "major" galaxies in the image have red shifts of about 280 to 295 million light years so it is likely this is about the correct distance to these two as well. IC 1505, the large elliptical like galaxy to the northwest has a red shift distance of 281 million light years. About all I find on it is are several comments that it is NOT Arp 295 as some authorities apparently claim. 2MASX J23420451-0334508 the spiral above the northern component of Arp 295 is at 296 million light years. There are three small galaxies directly west of the southern component. The faintest and furthest west is GALEX 2502913013803127866 an X ray galaxy at 291 million light years. The middle one is APMUKS(BJ) B233906.66-035605.1 at 284 million light years and the eastern galaxy is MRK 0933, a compact galaxy at 285 million light years. The face on spiral at the top of the image is APMUKS(BJ) B233913.30-034624.3 at 298 million light years. The apparent edge on blue galaxy to its east (left) is APMUKS(BJ) B233934.16-034639.4 at 296 million light years. While the elliptical southwest of the face on spiral and northwest of IC 1505 is 2MASX J23412885-0331266 at 288 million light years. The face on spiral nearly due west (right) of the lower component of Arp 295 is 2MASX J23411291-0337538 at 295 million light years. Not all galaxies in the image are members of the group. At the top of the image directly above the near edge on blue galaxy APMUKS(BJ) B233934.16-034639.4 is 2MASX J23420657-0328278 at 1.5 billion light years. To its east (left) just above my image but coming into it as a fuzzy halo is 2MASX J23422688-0327555 at 620 million light years. There are 4 asteroids in the image. The faintest is closest to Arp 295 about half way between the northern component and IC 1505. It is (186080) 2001 SO230 at magnitude 19.2. Above it and slightly left is the brightest asteroid, 220052) 2002 RY101 at 18.0. Above IC 1505 and level with the face on spiral near the top of the image is 2002 TD17 at magnitude 18.7. These last two are moving only in right ascension which is rare. The final asteroid slightly below center near the right edge. It is (136974) 1998 RO50 at magnitude 18.2. The reason the asteroids are sending a sloppy "A" in International Morris Code is that I took 6 frames but the second was lost to clouds. That created a gap in the trail but shows they were in retrograde motion moving west in the sky at the time I took the image. The "dot" is fainter than the rest of the trail as that image was partly lost to clouds as well. One advantage to not needing to guide is that you don't loose the target when clouds hit. It just picks up where you left off without me doing anything. In fact I was probably sound asleep when it happened. The night was very hazy with lots of gunk over the lake that I was imaging through. This created nasty halos about many stars. Seeing this when I started I set the system for 6 rather than my normal 4 Lumanosity and 4 rather than my normal 2 for color data but clouds wiped out one L and the last two red and first two green images. I really need to redo this one this fall under better skies. This field is out of the Sloan survey area but I did find a shot of this group taken by the one meter scope at the Naval Observatory in Flagstaff. Note they put the distance at 250 million light years. I don't know how this was determined. http://apod.nasa.gov/apod/ap051008.html Arp's image: http://nedwww.ipac.caltech.edu/level...ig_arp295.jpeg 14" LX200R @ f/10, L=5x10' RG=2x10'x3 B=4x10'x3, STL-11000XM, Paramount ME Rick -- Correct domain name is arvig and it is net not com. Prefix is correct. Third character is a zero rather than a capital "Oh". |
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ASTRO: Arp 295 a Zwicky connected system
"Stefan Lilge" wrote in news:7aK1o.227054$_F1.71925
@hurricane: Wow, that's what I call a tidal tail. I wonder if the straightness of the tail is caused by our angle of view or if it is real... Anyone living in that tail must have pretty boring skies. Poor folks. Brian -- http://www.skywise711.com - Lasers, Seismology, Astronomy, Skepticism Seismic FAQ: http://www.skywise711.com/SeismicFAQ/SeismicFAQ.html Quake "predictions": http://www.skywise711.com/quakes/EQDB/index.html Sed quis custodiet ipsos Custodes? |
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