ASTRO: Arp 305

Arp 305 is a pair of galaxies. That's how Arp classified them as well,
"Group Character: Double Galaxies. This is the same as Arp 303 I posted
a few days ago though this pair is really interesting. The northern
galaxy is NGC 4016. It looks to me as if it has two sets of spiral
arms. One set narrow and looping back to the core like a pretzel while
the other pair are broad and set at nearly a right angle to the first
pair. Both are obviously due to tidal effects of a close encounter,
probably with NGC 4017. But explaining their vast difference would seem
to me to be a major headache. Could it be two merged or superimposed
galaxies? If so rotational rates would likely be different but since we
see it so face on, likely not enough different to be measurable. NGC
4016 is classed by NED as SBdm:. Train-wreck is likely a better
classification. One note at NED says of it: "Distorted, patchy, hints
of spiral structure in the outskirts". Odd but I thought those arms
were rather obvious. Why it isn't classed as peculiar as well I can't
fathom. NGC project though does class it SBc-Irr which makes more sense
to me.

NGC 4017, while at first appearing more "normal" shows strong signs of
interaction with NGC 4016, not the least of which is the faint
connection that seems to run from its northern arm up to NGC 4016. Most
obvious is the debris almost dead center between them. It seems a bit
"windswept" (to use an Arp term) with whisps of stars appearing to have
been "blown" northwestward. Arp commented on this filament when he
said: "Segment breaking from arm of small galaxy, weak filaments reach
to north galaxy, which has figure 8 loops." The detached piece plus the
faint piece half way between almost make it look like the northern arm
of NGC 4017 is shooting star blobs at its companion. Note too that
there's a lot of debris off the southern arm as well that heads nearly
due east. I've attached a 150% enlargement of my image that shows this
a bit better than the main image. I suppose any residents living on
stars orbiting these detached pieces would resent being called debris.

The pair are located about 170 million light-years from us. NGC 4016 is
located about 2/3rds of a degree south of the southern border of Ursa
Major only a few seconds of arc into Coma Berenices from Leo. About 10
minutes of arc north of my image is the center of the NGC 4008 group.
This group is listed in NED to be about 170 million light-years distant.
It is likely Arp 305 is part of the group. Not far from its center is
NGC 4004 which is also highly distorted and on my list for next spring.
It too is 170 million light-years away and may have tangled with Arp 305.

The galaxy northwest of NGC 4016 is MAPS-NGP O_320_0562408. It's red
shift indicates a distance of only 40 million light-years. If so, it is
a dwarf irregular galaxy.

Well below NGC 4016 and southwest of NGC 4017 is a small lenticular
like, very red galaxy. It is SDSS J115824.86+272340.4 at just under 2
billion light-years. West of it is a blue star, angle up a bit from it
toward the very bright blue star, about one third of the way you come to
a smaller reddish galaxy, it too is 2 billion light-years away. It is
not an IR galaxy like the previous one was and not as red. It is SDSS
J115808.00+272428.4.

Southeast of NGC 4017 are two short dashes with a gap between them.
This is the asteroid (84842) 2003 AS17 at magnitude 19.1. I took color
data between two 20 minute luminosity imaging runs. That created the
gap as there's nothing for the color data to color in the gap. Below
the western end of the western trail is a very red spherical galaxy. It
is SDSS J115903.15+272321.9 and is also just under 2 billion light-years
from us. There are quite a few other galaxies in the lower part of the
frame that are at this 2 billion light year distance. 2 minutes of arc
below the south edge of the image almost on its centerline is the galaxy
cluster MaxBCG J179.60472+27.27528 with 22 members per NED. Its
distance is listed as, you guessed it, just under 2 billion light-years.
With no size given for it I can't tell if the 2 billion light-year
distant galaxies in my image are part of the group or not. It seems
likely however.

The fuzzy galaxy in the lower right corner is MAPS-NGP O_320_0562408.

SDSS image
http://astronomerica.awardspace.com/SDSS-30/NGC4016.php
http://astronomerica.awardspace.com/SDSS-30/NGC4017.php

Arp's image
http://nedwww.ipac.caltech.edu/level...ig_arp305.jpeg

14" LX200R @ f/10, L=4X10' RGB=2X10', 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".

Now that's a nice one, went straight to my harddisk.

Stefan

"Rick Johnson" schrieb im Newsbeitrag
. com...
Arp 305 is a pair of galaxies. That's how Arp classified them as well,
"Group Character: Double Galaxies. This is the same as Arp 303 I posted
a few days ago though this pair is really interesting. The northern
galaxy is NGC 4016. It looks to me as if it has two sets of spiral
arms. One set narrow and looping back to the core like a pretzel while
the other pair are broad and set at nearly a right angle to the first
pair. Both are obviously due to tidal effects of a close encounter,
probably with NGC 4017. But explaining their vast difference would seem
to me to be a major headache. Could it be two merged or superimposed
galaxies? If so rotational rates would likely be different but since we
see it so face on, likely not enough different to be measurable. NGC
4016 is classed by NED as SBdm:. Train-wreck is likely a better
classification. One note at NED says of it: "Distorted, patchy, hints
of spiral structure in the outskirts". Odd but I thought those arms
were rather obvious. Why it isn't classed as peculiar as well I can't
fathom. NGC project though does class it SBc-Irr which makes more sense
to me.

NGC 4017, while at first appearing more "normal" shows strong signs of
interaction with NGC 4016, not the least of which is the faint
connection that seems to run from its northern arm up to NGC 4016. Most
obvious is the debris almost dead center between them. It seems a bit
"windswept" (to use an Arp term) with whisps of stars appearing to have
been "blown" northwestward. Arp commented on this filament when he
said: "Segment breaking from arm of small galaxy, weak filaments reach
to north galaxy, which has figure 8 loops." The detached piece plus the
faint piece half way between almost make it look like the northern arm
of NGC 4017 is shooting star blobs at its companion. Note too that
there's a lot of debris off the southern arm as well that heads nearly
due east. I've attached a 150% enlargement of my image that shows this
a bit better than the main image. I suppose any residents living on
stars orbiting these detached pieces would resent being called debris.

The pair are located about 170 million light-years from us. NGC 4016 is
located about 2/3rds of a degree south of the southern border of Ursa
Major only a few seconds of arc into Coma Berenices from Leo. About 10
minutes of arc north of my image is the center of the NGC 4008 group.
This group is listed in NED to be about 170 million light-years distant.
It is likely Arp 305 is part of the group. Not far from its center is
NGC 4004 which is also highly distorted and on my list for next spring.
It too is 170 million light-years away and may have tangled with Arp 305.

The galaxy northwest of NGC 4016 is MAPS-NGP O_320_0562408. It's red
shift indicates a distance of only 40 million light-years. If so, it is
a dwarf irregular galaxy.

Well below NGC 4016 and southwest of NGC 4017 is a small lenticular
like, very red galaxy. It is SDSS J115824.86+272340.4 at just under 2
billion light-years. West of it is a blue star, angle up a bit from it
toward the very bright blue star, about one third of the way you come to
a smaller reddish galaxy, it too is 2 billion light-years away. It is
not an IR galaxy like the previous one was and not as red. It is SDSS
J115808.00+272428.4.

Southeast of NGC 4017 are two short dashes with a gap between them.
This is the asteroid (84842) 2003 AS17 at magnitude 19.1. I took color
data between two 20 minute luminosity imaging runs. That created the
gap as there's nothing for the color data to color in the gap. Below
the western end of the western trail is a very red spherical galaxy. It
is SDSS J115903.15+272321.9 and is also just under 2 billion light-years
from us. There are quite a few other galaxies in the lower part of the
frame that are at this 2 billion light year distance. 2 minutes of arc
below the south edge of the image almost on its centerline is the galaxy
cluster MaxBCG J179.60472+27.27528 with 22 members per NED. Its
distance is listed as, you guessed it, just under 2 billion light-years.
With no size given for it I can't tell if the 2 billion light-year
distant galaxies in my image are part of the group or not. It seems
likely however.

The fuzzy galaxy in the lower right corner is MAPS-NGP O_320_0562408.

SDSS image
http://astronomerica.awardspace.com/SDSS-30/NGC4016.php
http://astronomerica.awardspace.com/SDSS-30/NGC4017.php

Arp's image
http://nedwww.ipac.caltech.edu/level...ig_arp305.jpeg

14" LX200R @ f/10, L=4X10' RGB=2X10', 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".