Physics
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..396..381z&link_type=abstract
Formation and Evolution of Galaxy Disks ASP Conference Series, Vol. 396, Proceedings of the conference held 1-5 October, 2007 at
Physics
Scientific paper
We present a scaling relation that is satisfied by all classes of galaxies, ranging from dwarf spheroidals to brightest cluster galaxies and from disks to spheroidals, log r_{e} - log V^2 + log I_{e} + log Υ_{e} + 0.8 = 0, where r_{e} is the half light radius in kpc, V is a measure of the internal kinematics in km/sec, I_{e} is the surface brightness within r_{e} in L_&sun; pc^{-2}, and Υ_{e} is the I-band mass to light ratio within r_{e}. The low scatter with which galaxies lie about this relationship (0.09 dex) implies a regularity among galaxies that is encouraging to those attempting to uncover the basic physics of galaxy formation and places disk galaxies within the context of all galaxies.
Gonzalez Anthony H.
Zabludoff Ann I.
Zaritsky Dennis
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