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"NV" == Nicolaas Vroom writes:
NV "Joseph Lazio" schreef in bericht NV ... "JR" == Jeff Root writes: My recollection of rotation curves is such as those shown by Kent (Figure 1, URL: http://adsbit.harvard.edu/cgi-bin/np...J.....93..816K ). NV This document at page 5 = page 821 shows the following sentence: NV "In principle, the bulge and the disk must be treated differently NV since they contribute in different ways to the rotation curve" Why NV differently ? What is meant with: "different ways" In principle NV the rotation curve at each distance r from the center of the NV galaxy depents on the mass dm at each position x,y,z I don't have my copy of Binney & Tremaine in front of me, but I have a dim recollection that the gravitational potential of a disk is different than that of a spherical distribution. That has an impact on the rotation curve. See URL:http://www.astro.su.se/%7Epawel/gradprobl.2.html for examples. NV Next they write: "Also they are likely to have different M/L NV ratios" Why ? NV IMO it is not so strange that M/L ratios are different but if that NV is the case and when there is a disk it becomes more difficult to NV calculate the mass of the disk accurately. The stars are different. Bulges are dominated by low-mass stars, comparable to the Sun. Most of the light from a disk comes from the high-mass stars (which are absent in a bulge), but the high-mass stars contribute very little to the overall mass of the disk. (A 10 solar mass star might have a luminosity of 100 solar luminosities.) -- Lt. Lazio, HTML police | e-mail: No means no, stop rape. | http://patriot.net/%7Ejlazio/ sci.astro FAQ at http://sciastro.astronomy.net/sci.astro.html |
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