... This will be an interesting object to see if any galaxies were actually detected in the UV has the center of coma is a very dense region and home to old, dead galaxies. ...
... On the scale of the Galaxy however, there is rather direct evidence for nun-luminous ... If light traces mass in a galaxy then we expect a kelperian fall off in rotational ... This is never observed in any galaxy: . Some sample rotation curves: . ...
... There do not appear to be many, red, spherical galaxies that might be identified as distant elliptical galaxies. ... This is consistent with the notion that elliptical galaxies form as the result of the merger of spiral galaxies. ...
... galaxy, as outlined by these two different age stellar populations, should be ... resolution this galaxy is well resolved into stars which indicates the galaxy to ... a very diffuse galaxy, similar to the low surface brightness galaxy shown in figure ...
... The velocity of the galaxy would then be 300,000 x .005 = 1500 km/s. In addition, some galaxies have emission lines that are principally due to hydrogren recombination. ...
... galaxies in the near-UV in comparison with ground-based optical observations. to extend the wavelength coverage over which colors are determined and to see if there is any near-UV bright component that may help to explain the observ ed blue colors in ...
... The face-on orientation of the galaxy means that obscuration by dust in the galaxy is minimal. ... NGC 5253 is a peculiar low mass spiral galaxy in the nearby Centaurus group of galaxies. ...