A relation between the characteristic stellar ages of galaxies and their intrinsic shapes-Reference-Cited by-同舟云学术

A relation between the characteristic stellar ages of galaxies and their intrinsic shapes

Published:2018-04-23 Issue:6 Volume:2 Page:483-488
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

van de Sande Jesse^ORCID,Scott Nicholas^ORCID,Bland-Hawthorn Joss,Brough Sarah,Bryant Julia J.,Colless Matthew,Cortese Luca,Croom Scott M.,d′Eugenio Francesco,Foster Caroline,Goodwin Michael,Konstantopoulos Iraklis S.,Lawrence Jon S.,McDermid Richard M.,Medling Anne M.,Owers Matt S.,Richards Samuel N.,Sharp Rob

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://www.nature.com/articles/s41550-018-0436-x.pdf

Reference53 articles.

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3. Bender, R., Burstein, D. & Faber, S. M. Dynamically hot galaxies. II. Global stellar populations. Astrophys. J. 411, 153–169 (1993).

4. Cappellari, M. Structure and kinematics of early-type galaxies from integral field spectroscopy. Annu. Rev. Astron. Astrophys. 54, 597–665 (2016).

5. Naab, T. et al. The ATLAS3D project—XXV. Two-dimensional kinematic analysis of simulated galaxies and the cosmological origin of fast and slow rotators. Mon. Not. R. Astron. Soc. 444, 3357–3387 (2014).

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