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The Evolution of Spiral Disks

Matthew A. Bershady·David R. Andersen
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Abstract

We report on aspects of an observational study to probe the mass assembly of large galaxy disks. In this contribution we focus on a new survey of integral-field H-alpha velocity-maps of nearby, face on disks. Preliminary results yield disk asymmetry amplitudes consistent with estimates based on the scatter in the local Tully-Fisher relation. We also show how the high quality of integral-field echelle spectroscopy enables determinations of kinematic inclinations to i~20 deg. This holds the promise that nearly-face-on galaxies can be included in the Tully-Fisher relation. Finally, we discuss the prospects for measuring dynamical asymmetries of distant galaxies.

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Matthew A. Bershady, David R. Andersen. 1999-10-15. The Evolution of Spiral Disks. https://arxiv.org/abs/astro-ph/9910281

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