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Hα kinematics of nearby galaxies using Fabry-Perot and IFU data

Published online by Cambridge University Press:  21 March 2017

Santiago Erroz-Ferrer  and
the S4G Team and the MUSE-GTO Consortium
Santiago Erroz-Ferrer
Affiliation:
Instituto de Astrofisica de Canarias, Via Lactea s/n 38205 La Laguna, Spain email: [email protected] Departamento de Astrofisica, Universidad de La Laguna, Avda. Astrofisico Francisco Sanchez s/n 38206 La Laguna, Spain Department of Physics, Institute for Astronomy, ETH Zurich, CH-8093 Zurich, Switzerland
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Abstract

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I present here analysis of the shapes of the rotation curves of a large sample of nearby spiral galaxies with high angular and spectral resolution Hα (Fabry-Perot GHαFaS) kinematics, and the resulting constraints on their total mass distributions. In particular I discuss how their rotation curve shapes relate to key galaxy properties. Finally I present related results from the MUSE Atlas of Disks (MAD) program, which is dissecting the nearby disk population with IFU spectroscopy at ~100pc resolution.

Keywords

Spirals - kinematics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S321: Formation and Evolution of Galaxy Outskirts , March 2016 , pp. 275
Copyright
Copyright © International Astronomical Union 2017 

References

Erroz-Ferrer, S., Knapen, J. H., Leaman, R., et al. 2016, MNRAS, 458, 1119 Google Scholar