Optical integral field spectroscopy observations applied to simulated galaxies: testing the fossil record method
Author:
Affiliation:
1. Instituto de Astronomía, Universidad Nacional Autónoma de México, A.P. 70-264, 04510 CDMX, México
2. Instituto de Radioastronomía y Astrofísica, Universidad Nancional Autónoma de México, Box 70-3, Morelia, Michoacán, México
Funder
Division of Atmospheric and Geospace Sciences
Center for Computing for Life Sciences, San Francisco State University
Alfred P. Sloan Foundation
U.S. Department of Energy
University of Arizona
University of Colorado Boulder
University of Oxford
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/483/4/4525/27379058/sty3256.pdf
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4. Kinematic scaling relations of CALIFA galaxies: A dynamical mass proxy for galaxies across the Hubble sequence
5. THE SPECIFIC STAR FORMATION RATE AND STELLAR MASS FRACTION OF LOW-MASS CENTRAL GALAXIES IN COSMOLOGICAL SIMULATIONS
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