Morphology rather than environment drives the SFR–mass relation in the local universe-Reference-Cited by-同舟云学术

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Morphology rather than environment drives the SFR–mass relation in the local universe

Published:2018-09-14 Issue:3 Volume:481 Page:3456-3469
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Calvi R¹²,Vulcani B³⁴^ORCID,Poggianti B M⁴,Moretti A⁴,Fritz J⁵,Fasano G⁴

Affiliation:

1. Instituto de Astrofísica de Canarias, E-38200 La Laguna, Spain

2. Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Spain

3. School of Physics, University of Melbourne, VIC 3010, Australia

4. INAF – Astronomical Observatory of Padova, I-35122 Padova, Italy

5. Instituto de Radioastronomía y Astrofísica, IRyA, UNAM, Campus Morelia, A.P. 3-72, C.P. 58089, Mexico

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/481/3/3456/25838563/sty2476.pdf

Reference119 articles.

1. THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY

2. THE MASS-INDEPENDENCE OF SPECIFIC STAR FORMATION RATES IN GALACTIC DISKS

3. The Fifth Data Release of the Sloan Digital Sky Survey

4. DIFFERENCES IN THE STRUCTURAL PROPERTIES AND STAR FORMATION RATES OF FIELD AND CLUSTER GALAXIES AT Z ∼ 1

5. Evidence for systematic evolution in the properties of galaxies in distant clusters

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3. Galaxy Clusters from the DESI Legacy Imaging Surveys. II. Environmental Effects on the Size–Mass Relation;The Astrophysical Journal;2024-01-31

4. A Census of Star Formation Histories of Massive Galaxies at 0.6 < z < 1 from Spectrophotometric Modeling Using Bagpipes and Prospector;The Astrophysical Journal;2024-01-01

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