Other
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...20314608w&link_type=abstract
American Astronomical Society Meeting 203, #146.08; Bulletin of the American Astronomical Society, Vol. 36, p.591
Other
Scientific paper
Radial color gradients provide powerful diagnostics for understanding the spatio-temporal histories of star formation in disk galaxies. The long baselines in wavelength spanned by (UV - Opt) colors lead to especially sensitive indices of composite stellar population and corresponding starbirth history. We examine the (UV - Opt) radial color gradients in nearby giant and dwarf disk galaxies that were published in Marcum et al. (2001), Kuchinski et al. (2000), and Stewart (2000; 1998) based on data obtained with the space shuttle-borne Ultraviolet Imaging Telescope (UIT) and various optical telescopes. Several well-known giant disk galaxies (e.g. M31, M33, M81) show significant blueing with increasing radius. These radial color gradients imply that the galaxian disks are evolving from the inside out. Other giant disk galaxies (M51, M74, M83) show a two-step blueing from the inner to the outer disk. Still other giant spirals (M77, NGC 2903, NGC 4321) are remarkably constant in (UV - Opt) color. Starbursting rings (in M94, NGC 1097, NGC 1317) are clearly evident as UV-bright enhancements. Irregular and dwarf disk galaxies show both radial blueing (Holmberg II), constant (NGC 4449), and reddening (NGC 4214) behavior. We attempt to make some sense out of this intriguing diversity in radial color gradients.
Fanelli Michael N.
Marcum Pamela Marie
Stewart Susan G.
Waller William H.
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