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25 April 2024

» arxiv » astro-ph/0609436

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Ongoing Formation of Bulges and Black Holes in the Local Universe: New Insights from GALEX
Guinevere Kauffmann ; Timothy M. Heckman ; Tamas Budavari ; Stephane Charlot ; Charles G. Hoopes ; D. Christopher Martin ; Mark Seibert ; Tom A. Barlow ; Luciana Bianchi ; Tim Conrow ; Jose Donas ; Karl Forster ; Peter G. Friedman ; Young-Wook Lee ; Barry F. Madore ; Bruno Milliard ; Patrick F. Morrissey ; Susan G. Neff ; R. Michael Rich ; David Schiminovich ; Todd Small ; Alex S. Szalay ; Ted K. Wyder ; S.K. Yi ;
Date:	15 Sep 2006
Abstract:	We analyze a volume-limited sample of massive bulge-dominated galaxies with data from both the Sloan Digital Sky Survey and the Galaxy Evolution Explorer (GALEX) satellite. The galaxies have central velocity dispersions greater than 100 km/s and stellar surface mass densities that lie above the value where galaxies transition from actively star forming to passive systems. The sample is limited to redshifts 0.03<z<0.07. At these distances, the SDSS spectra sample the light from the bulge-dominated central regions of the galaxies. The GALEX NUV data provide high sensitivity to low rates of global star formation in these systems. Our sample of bulge-dominated galaxies exhibits a much larger dispersion in NUV-r colour than in optical g-r colour. Nearly all of the galaxies with bluer NUV-r colours are AGN. Both GALEX images and SDSS colour profiles demonstrate that the excess UV light is associated with an extended disk. We find that galaxies with red outer regions almost never have a young bulge or a strong AGN. Galaxies with blue outer regions have bulges and black holes that span a wide range in age and accretion rate. Galaxies with young bulges and strongly accreting black holes almost always have blue outer disks. Our suggested scenario is one in which the source of gas that builds the bulge and black hole is a low mass reservoir of cold gas in the disk.The presence of this gas is a necessary, but not sufficient condition for bulge and black hole growth. Some mechanism must transport this gas inwards in a time variable way. As the gas in the disk is converted into stars, the galaxies will turn red, but further gas infall can bring them back into the blue NUV-r sequence.(Abridged)
Source:	arXiv, astro-ph/0609436
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