The unexpectedly large dust and gas content of quiescent galaxies at z

The unexpectedly large dust and gas content of quiescent galaxies at z > 1.4

Published:2018-01-15 Issue:3 Volume:2 Page:239-246
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Gobat R.^ORCID,Daddi E.,Magdis G.,Bournaud F.,Sargent M.,Martig M.,Jin S.,Finoguenov A.,Béthermin M.,Hwang H. S.,Renzini A.,Wilson G. W.,Aretxaga I.,Yun M.,Strazzullo V.,Valentino F.

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://www.nature.com/articles/s41550-017-0352-5.pdf

Reference105 articles.

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2. Sargent, M. T. et al. A direct constraint on the gas content of a massive, passively evolving elliptical galaxy at z = 1.43. Astrophys. J. Lett. 806, 6 (2015).

3. Gobat, R. et al. The early early type: discovery of a passive galaxy at z spec ~ 3. Astrophys. J. Lett. 759, 5 (2012).

4. Glazebrook, K. et al. A massive, quiescent galaxy at redshift of z = 3.717. Nature 544, 71–74 (2017).

5. Di Matteo, T., Springel, V. & Hernquist, L. Energy input from quasars regulates the growth and activity of black holes and their host galaxies. Nature 433, 604–607 (2005).

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