Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang

Author:

Tacchella S.1,Carollo C. M.1,Renzini A.2,Schreiber N. M. Förster3,Lang P.3,Wuyts S.3,Cresci G.4,Dekel A.5,Genzel R.367,Lilly S. J.1,Mancini C.2,Newman S.6,Onodera M.1,Shapley A.8,Tacconi L.3,Woo J.1,Zamorani G.9

Affiliation:

1. Department of Physics, Institute for Astronomy, ETH Zurich, CH-8093 Zurich, Switzerland.

2. Istituto Nazionale di Astrofisica (INAF) Osservatorio Astronomico di Padova, Vicolo dell Osservatorio 5, I-35122 Padova, Italy.

3. Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, Germany.

4. INAF Osservatorio Astronomico di Arcetri, Largo Enrico Fermi 5, I-50125 Firenze, Italy.

5. Racah Institute of Physics, The Hebrew University, Jerusalem 91904, Israel.

6. Department of Astronomy, Campbell Hall, University of California, Berkeley, CA 94720, USA.

7. Department of Physics, Le Conte Hall, University of California, Berkeley, CA 94720, USA.

8. Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1547, USA.

9. INAF Osservatorio Astronomico di Bologna, Via Ranzani 1, I-40127 Bologna, Italy.

Abstract

Eat your heart out, old galaxies Most galaxies exceeding 100 billion solar masses are dense spheroids that exhibit no star-forming activity in the present day. Nevertheless, galaxies of the same size were actively forming stars when the universe was only a few billion years old. Tacchella et al. used integral-field spectroscopy and high-resolution imaging to map the distributions of star formation rates and stellar mass densities within ancient galaxies. Star formation apparently quenched first in the center, while remaining lively in the galactic outskirts, with quenching taking a few billion years to proceed outward. Science , this issue p. 314

Funder

Swiss National Science Foundation

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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