The Stability of Galaxy Disks

Kyle B. Westfall, D. R. Andersen, M. A. Bershady, T. Martinsson, R. A. Swaters, M. A. Verheijen

Research output: Chapter in Book/Report/Conference proceedingConference contributionAcademicpeer-review

Abstract

Using measurements of velocity dispersion and mass surface density for both the gas and stellar components, we calculate the multi-component stability (Q) for 30 galaxy disks observed by the DiskMass Survey. Despite their sub-maximality (Bershady et al. 2011, ApJL, 739, 47), we find all disks to be stable with roughly 85% falling in the range 1
Original languageEnglish
Title of host publicationAmerican Astronomical Society Meeting Abstracts
Pages146.15
Publication statusPublished - Jan-2013
EventAmerican Astronomical Society, AAS Meeting #221, #146.15 - Long Beach, California, United States
Duration: 6-Jan-201310-Jan-2013

Conference

ConferenceAmerican Astronomical Society, AAS Meeting #221, #146.15
Country/TerritoryUnited States
CityLong Beach, California
Period06/01/201310/01/2013

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