|
|
Thread Tools | Display Modes |
#61
|
|||
|
|||
Galaxies without dark matter halos?
wrote in message
... On Thu, 25 Sep 2003, greywolf42 wrote: -- I believe the original set of luminosity and galaxy type was built by using distances determined with the Hubble redshift method. If by "the original set" you mean something like "The original set that Hubble made" (or other decades old set), so what? It's not in use now and the Hubble relation is still there. If you mean that the Hubble constant is used the calibrate, say, Tully-Fischer *TODAY* -That- -is- -*still*- -just- -flat- -wrong-. As an almost trivial amount of reading would show you. People in fact calibrate T-F with different methods just to compare the results. Then what is used? Why simply assert that I'm wrong? Why not mention the physical process used to calibrate Tully-Fischer? A list from an introductory text does not provide all the information required to address the issue. It does, however, point out how easy it would be for you to find such information -if- you wanted to. Since you now imply that such intro texts are too basic should I revert to an obvious reason other than lack of knowledge why you would make an incorrect statement? And I still recommend you read Shu. Why add another text, since you apparently don't know what the reason is yourself? My point was that the (local) Cepheid galaxies are the primary basis of the Hubble distance relation. If that is you point, say it, not somthing else. I did say it. But even if the Chepeid distance is off by a factor of a million: "Still it moves" --A plot of distance vs. redshift which is linear in ly vs delta l/l is still linear when re-labeled parsecs vs. delta l/l or cm or teraparsecs. How does this relate to the calibration of the Tully-Fischer scaling law? To generalize my point, using your classification scheme, the intermermediate and global distance relationships (except for the supernovae) were all founded on distances that were based on the Hubble constant. But this is not true. I measure the distance to some galaxies using Cepheids & RR Lyae. RR Lyrae stars are less luminous that Cepheids. Hence Cepheids determine the maximum distance to which we have a non-redshift-based correlation. I measure the 21cm line of these galaxies. I do a regression of distance vs. line width. I measure the 21cm line width of a new galaxie and use my regression result to calculate the distance. I have not even measured a red shift yet, so how am I possibly using the Hubble relation?? Because you are making the theoretical assumption that the cause of the change in line width is velocity of the galaxy. Just like the assumption that the cause of the hubble shift is velocity. Which is why the universal distance scale shifted when Hipparcos was actually able to measure the parallax of a Cepheid variable star. Hipparcos found that Cepheids were closer than theoretically expected. Which shifted 'in' the two dozen baseline galaxies. Which shifted the Hubble constant. Which 'shrank' the rest of the universe. Again, so what? In fact no, not "So what" --they corrected the error and changed the distances. Something you repeatedly imply they don't do. The point is, that if the long distance range was not based solely on the hubble relation, then shifting in the 'hubble' galaxies would not have affected the long distance scales. Because those 'other' methods wouldn't change. People have cross compared these where ever it makes sense. They know when calibrating method A from method B and Method C from B errors build up, both statistical & flaws in the methods. That is why you see them delighted that -different- methods agree. And most importantly, even if you do prove the units are wrong the distance-redshift relation doesn't go away. I have no idea why you think this is important, because I never claimed or implied that the discussion was over 'units.' Nor did I imply that there is no distance-redshift relationship in the nearer galaxies. I once saw a plot of a set of random* galaxies plotted appearant size vs. redshift. There was a Hubble law. I presume you mean that they used the hubble constant to determine the distances to those random galaxies. If you can, explain it some nonstandard way, but denial or misrepresentation of the observations or observational methods isn't going to work. Explain what? I've never denied the observations or the methods. I've merely tried to point out to you that the conversion of the observations to conclusions about distance in the far field are all based on the theoretical assumption of the big bang. Hence, one cannot use these observations themselves as support for the big bang -- because the distance were all determined from that assumption. greywolf42 ubi dubium ibi libertas |
#62
|
|||
|
|||
Galaxies without dark matter halos?
In article , greywolf42
writes: The "dogma" has changed, motivated almost entirely by data. No-one ever suggested that Omega was 0.3 and lambda 0.7 based on anything except data. Thus, I would argue that the current standard model is primarily data driven. Just because someone mistakenly elevates it to dogma doesn't make it automatically wrong. Dogma is not automatically wrong. (Just ask of the various churches.) However, dogma is primarily of theoretical origin (or theological origin -- sometimes it's hard to divorce the two). The two values you provided are based on the dogma that omega = 1.0. We both agree that there was and perhaps still might be a dogma stating that Omega_total (i.e. Omega_matter + lambda) must be 1, and that this dogma, when first developed, didn't have sufficient motivation. However, the values I mentioned above (0.7 and 0.3) are derived from observations whether or not one believes this dogma. The interesting question now is how close this sum is to 1: Within 10%? 1%? 0.1%? |
#63
|
|||
|
|||
Galaxies without dark matter halos?
In article , greywolf42
writes: The "dogma" has changed, motivated almost entirely by data. No-one ever suggested that Omega was 0.3 and lambda 0.7 based on anything except data. Thus, I would argue that the current standard model is primarily data driven. Just because someone mistakenly elevates it to dogma doesn't make it automatically wrong. Dogma is not automatically wrong. (Just ask of the various churches.) However, dogma is primarily of theoretical origin (or theological origin -- sometimes it's hard to divorce the two). The two values you provided are based on the dogma that omega = 1.0. We both agree that there was and perhaps still might be a dogma stating that Omega_total (i.e. Omega_matter + lambda) must be 1, and that this dogma, when first developed, didn't have sufficient motivation. However, the values I mentioned above (0.7 and 0.3) are derived from observations whether or not one believes this dogma. The interesting question now is how close this sum is to 1: Within 10%? 1%? 0.1%? |
#64
|
|||
|
|||
Galaxies without dark matter halos?
Ulf Torkelsson wrote in message
... There is no such theoretical relationship as you imagine. I wasn't the one that claimed there was. For most Hubble types you can find both small and large galaxies, and always there is a significant spread in the luminosities. You are correct, but -- again -- we aren't discussing the Hubble classification scheme. No, the Tully-Fisher scheme has never been calibrated based on the Hubble constant, that is plainly wrong. There are also more distance indicators than the Cepheids. Well, yes. But the Cepheids provide the largest non-redshift assumption distance scale. May I suggest that you pick up the book: Rowan-Robinson, M., 1985, The cosmological distance ladder, W. H. Freeman & Comp., New York Rowan-Robinson describes in detail how you build up the cosmological distance scale. You start with the primary indicators, cepheids, supernovae, novae and RR Lyrae variables. You then use these to calibrate new distance indicators, such as the size of HII-regions, globular clusters, the brightest stars in the galaxies, the Tully-Fisher relation and so on. In the end you can even use the brightest cluster galaxies to determine the distances to clusters of galaxies. Nowhere in this process do you use Hubble's constant. You use the hubble constant anywhere outside the range of Cepheids. The (fairly recent) supernovae calibrations were produced after all the others were (i.e. Tully-Fischer relation) were already "set." Indeed, with a publication date of 1985, the supernovae ladder won't be included. Next time I'm at the library, I check out Rowan-Robinson. greywolf42 ubi dubium ibi libertas [Mod. note: quoted text trimmed. Please do this yourself. I have begun rejecting, and will continue to reject, postings with excessive quoted text -- mjh] |
#65
|
|||
|
|||
Galaxies without dark matter halos?
Ulf Torkelsson wrote in message
... There is no such theoretical relationship as you imagine. I wasn't the one that claimed there was. For most Hubble types you can find both small and large galaxies, and always there is a significant spread in the luminosities. You are correct, but -- again -- we aren't discussing the Hubble classification scheme. No, the Tully-Fisher scheme has never been calibrated based on the Hubble constant, that is plainly wrong. There are also more distance indicators than the Cepheids. Well, yes. But the Cepheids provide the largest non-redshift assumption distance scale. May I suggest that you pick up the book: Rowan-Robinson, M., 1985, The cosmological distance ladder, W. H. Freeman & Comp., New York Rowan-Robinson describes in detail how you build up the cosmological distance scale. You start with the primary indicators, cepheids, supernovae, novae and RR Lyrae variables. You then use these to calibrate new distance indicators, such as the size of HII-regions, globular clusters, the brightest stars in the galaxies, the Tully-Fisher relation and so on. In the end you can even use the brightest cluster galaxies to determine the distances to clusters of galaxies. Nowhere in this process do you use Hubble's constant. You use the hubble constant anywhere outside the range of Cepheids. The (fairly recent) supernovae calibrations were produced after all the others were (i.e. Tully-Fischer relation) were already "set." Indeed, with a publication date of 1985, the supernovae ladder won't be included. Next time I'm at the library, I check out Rowan-Robinson. greywolf42 ubi dubium ibi libertas [Mod. note: quoted text trimmed. Please do this yourself. I have begun rejecting, and will continue to reject, postings with excessive quoted text -- mjh] |
#66
|
|||
|
|||
Galaxies without dark matter halos?
Phillip Helbig---remove CLOTHES to reply
wrote in message ... We both agree that there was and perhaps still might be a dogma stating that Omega_total (i.e. Omega_matter + lambda) must be 1, and that this dogma, when first developed, didn't have sufficient motivation. However, the values I mentioned above (0.7 and 0.3) are derived from observations whether or not one believes this dogma. My understanding of the source of the omega = 0.3 was the BB with Omega = 1.0. May I ask what sources for 0.3 and 0.7 are you using? The interesting question now is how close this sum is to 1: Within 10%? 1%? 0.1%? I belive it's as arbitrarily close as the assumptions in your calculations. greywolf42 ubi dubium ibi libertas [Mod. note: quoted text trimmed -- mjh] |
#67
|
|||
|
|||
Galaxies without dark matter halos?
Phillip Helbig---remove CLOTHES to reply
wrote in message ... We both agree that there was and perhaps still might be a dogma stating that Omega_total (i.e. Omega_matter + lambda) must be 1, and that this dogma, when first developed, didn't have sufficient motivation. However, the values I mentioned above (0.7 and 0.3) are derived from observations whether or not one believes this dogma. My understanding of the source of the omega = 0.3 was the BB with Omega = 1.0. May I ask what sources for 0.3 and 0.7 are you using? The interesting question now is how close this sum is to 1: Within 10%? 1%? 0.1%? I belive it's as arbitrarily close as the assumptions in your calculations. greywolf42 ubi dubium ibi libertas [Mod. note: quoted text trimmed -- mjh] |
#68
|
|||
|
|||
Galaxies without dark matter halos?
greywolf42 wrote:
Ulf Torkelsson wrote in message ... No, the Tully-Fisher scheme has never been calibrated based on the Hubble constant, that is plainly wrong. There are also more distance indicators than the Cepheids. Well, yes. But the Cepheids provide the largest non-redshift assumption distance scale. This is simply incorrect. The cepheids can be, and have been, used to calibrate other distance indicators such as the sizes of the largest HII-regions of the galaxies, the brightnesses and sizes of the brightest galaxies in clusters of galaxies, the Tully-Fisher relation and so on. None of these distance scales will then depend on the value of Hubble's constant as you have claimed. Ulf Torkelsson [Mod. note: reformatted -- mjh] |
#69
|
|||
|
|||
Galaxies without dark matter halos?
greywolf42 wrote:
Ulf Torkelsson wrote in message ... No, the Tully-Fisher scheme has never been calibrated based on the Hubble constant, that is plainly wrong. There are also more distance indicators than the Cepheids. Well, yes. But the Cepheids provide the largest non-redshift assumption distance scale. This is simply incorrect. The cepheids can be, and have been, used to calibrate other distance indicators such as the sizes of the largest HII-regions of the galaxies, the brightnesses and sizes of the brightest galaxies in clusters of galaxies, the Tully-Fisher relation and so on. None of these distance scales will then depend on the value of Hubble's constant as you have claimed. Ulf Torkelsson [Mod. note: reformatted -- mjh] |
#70
|
|||
|
|||
Galaxies without dark matter halos?
greywolf42 wrote:
Ulf Torkelsson wrote in message ... No, the Tully-Fisher scheme has never been calibrated based on the Hubble constant, that is plainly wrong. There are also more distance indicators than the Cepheids. Well, yes. But the Cepheids provide the largest non-redshift assumption distance scale. This is simply incorrect. The cepheids can be, and have been, used to calibrate other distance indicators such as the sizes of the largest HII-regions of the galaxies, the brightnesses and sizes of the brightest galaxies in clusters of galaxies, the Tully-Fisher relation and so on. None of these distance scales will then depend on the value of Hubble's constant as you have claimed. Ulf Torkelsson [Mod. note: reformatted -- mjh] |
Thread Tools | |
Display Modes | |
|
|
Similar Threads | ||||
Thread | Thread Starter | Forum | Replies | Last Post |
"Dark matter" forms dense clumps in ghost universe (Forwarded) | Andrew Yee | Astronomy Misc | 0 | November 21st 03 04:41 PM |
Galaxies without dark matter halos? | greywolf42 | Astronomy Misc | 34 | November 5th 03 12:34 PM |
A Detailed Map of Dark Matter in a Galactic Cluster Reveals How Giant Cosmic Structures Formed | Ron Baalke | Astronomy Misc | 3 | August 5th 03 02:16 PM |
Galaxies without dark matter halos? | Ed Keane III | Research | 4 | August 4th 03 12:39 PM |
Hubble tracks down a galaxy cluster's dark matter (Forwarded) | Andrew Yee | Astronomy Misc | 0 | July 17th 03 01:42 PM |