AAS 207th Meeting, 8-12 January 2006
Session 202 Galaxies and their Components
Oral, Thursday, 2:00-3:30pm, January 12, 2006, Virginia

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[202.02] Properties of Extended UV Disk (XUV-disk) Galaxies Discovered by GALEX

D. A. Thilker, L. Bianchi, G. Meurer (JHU), A. Gil de Paz, B. Madore, S. Boissier (OCIW), A. Ferguson (ROE), S. Hameed (Hampshire), GALEX Team

We have examined a sample of nearby spiral galaxies observed in the UV by GALEX for which H\alpha imaging is also available. Our study focused on the radial variation of star formation rate and surface covering factor of UV-bright complexes in the outer galactic disk, in the regime where star formation threshold mechanisms are vitally important. We suggest a classification scheme for identifying extended UV disks (XUV-disks, eg. Thilker et al. and Gil de paz et al.) in our sample, and use this method to constrain salient ensemble characteristics of this galaxy population. Approximately 20-30% of the galaxies in our sample exhibit XUV-disk emission, most frequently in mid-to-early type giant spirals and dwarf Magellanic type galaxies. Some of the XUV disks in our sample appear to have similarly extended H\alpha emission originating from sparsely distributed HII regions. We suggest that optically-identified, anti-truncated S0-Sb galaxies may represent the evolved (or presently quiescent) counterparts of the massive XUV-disk population. Finally, we utilize multiwavelength optical imaging in conjunction with our GALEX data for a few XUV-disk galaxies to constrain the stellar mass, bolometric luminosity, and age of individual stellar complexes in the outer disk environment.

We gratefully acknowledge NASA's support for construction, operation and data analysis of the GALEX mission, developed in cooperation with the French CNES and Korean Ministry of Science and Technology.

If you would like more information about this abstract, please follow the link to http://dolomiti.pha.jhu.edu/. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.

The author(s) of this abstract have provided an email address for comments about the abstract: dthilker@pha.jhu.edu

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