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28 March 2024
 
  » arxiv » astro-ph/0201407

 Article overview


WIYN Integral-Field Kinematics of Disk Galaxies
Matthew Bershady ; Marc Verheijen ; David Andersen ;
Date 24 Dec 2001
Subject astro-ph
AffiliationU of Wisconsin), David Andersen (MPIA, Heidelberg
AbstractWe have completed a new fiber array, SparsePak, optimized for low-surface-brightness studies of extended sources on the WIYN telescope. We are now using this array as a measuring engine of velocity and velocity-dispersion fields of stars and ionized gas in disk galaxies from high to low surface-brightness. Here we present commissioning data on the velocity ellipsoids, surface densities and mass-to-light ratios in two blue, high surface-brightness, yet small disks. If our preliminary results survive further observation and more sophisticated analysis, then NGC 3949 has sigma_z/sigma_R >> 1, implying strong vertical heating, while NGC 3982’s disk is substantially sub-maximal. These galaxies are strikingly unlike the Milky Way, and yet would be seen more easily at high redshift.
Source arXiv, astro-ph/0201407
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