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

Bibcode
2017IAUS..321..275E
DOI
10.1017/S1743921316009443
Erroz-Ferrer, S.; S4G Team; MUSE-GTO Consortium
Referencia bibliográfica

Formation and Evolution of Galaxy Outskirts, Proceedings of the International Astronomical Union, IAU Symposium, Volume 321, pp. 275-275

Advertised on:
3
2017
Número de autores
3
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
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.
Tipo
Sin árbitro

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