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Dynamical regularities in rotating galaxies

Published online by Cambridge University Press:  14 May 2020

Stacy McGaugh Open the ORCID record for Stacy McGaugh [Opens in a new window] ,
Federico Lelli ,
Pengfei Li  and
Jim Schombert
Stacy McGaugh
Affiliation:
Department of Astronomy, Case Western Reserve University, Cleveland, OH44106, USA
Federico Lelli
Affiliation:
European Southern Observatory, 85748, Garching bei München, Germany
Pengfei Li
Affiliation:
Department of Astronomy, Case Western Reserve University, Cleveland, OH44106, USA
Jim Schombert
Affiliation:
Department of Physics, University of Oregon, Eugene, OR97403, USA
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Abstract

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Galaxies are observed to obey a strict set of dynamical scaling relations. We review these relations for rotationally supported disk galaxies spanning many decades in mass, surface brightness, and gas content. The behavior of these widely varied systems can be summarized with a handful of empirical laws connected by a common acceleration scale.

Keywords

galaxies: dwarfgalaxies: irregulargalaxies: kinematics and dynamicsgalaxies: spiralgalaxies: structure
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S353: Galactic Dynamics in the Era of Large Surveys , June 2019 , pp. 144 - 151
Copyright
© International Astronomical Union 2020

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