Evolution of spatially resolved star formation main sequence and surface density profiles in massive disc galaxies at 0 ≲ z ≲ 1: inside–out stellar mass buildup and quenching-Reference-Cited by-同舟云学术

Evolution of spatially resolved star formation main sequence and surface density profiles in massive disc galaxies at 0 ≲ z ≲ 1: inside–out stellar mass buildup and quenching

Published:2018-07-04 Issue:4 Volume:479 Page:5083-5100
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Abdurro’uf ¹,Akiyama Masayuki¹

Affiliation:

1. Astronomical Institute, Tohoku University, Aramaki, Aoba, Sendai 980-8578, Japan

Funder

National Aeronautics and Space Administration

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/479/4/5083/25207642/sty1771.pdf

Reference66 articles.

1. Understanding the scatter in the spatially resolved star formation main sequence of local massive spiral galaxies

2. Must Star-forming Galaxies Rapidly Get Denser before They Quench?

3. SDSS IV MaNGA – sSFR profiles and the slow quenching of discs in green valley galaxies

4. SExtractor: Software for source extraction

5. Virial shocks in galactic haloes?

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