The ALMaQUEST survey - III. Scatter in the resolved star-forming main sequence is primarily due to variations in star formation efficiency Article

Ellison, Sara L, Thorp, Mallory D, Lin, Lihwai et al. (2020). The ALMaQUEST survey - III. Scatter in the resolved star-forming main sequence is primarily due to variations in star formation efficiency . MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 493(1), L39-L43. 10.1093/mnrasl/slz179

Open Access International Collaboration

cited authors

  • Ellison, Sara L; Thorp, Mallory D; Lin, Lihwai; Pan, Hsi-An; Bluck, Asa FL; Scudder, Jillian M; Teimoorinia, Hossen; Sanchez, Sebastian F; Sargent, Mark

authors

publication date

  • March 1, 2020

published in

keywords

  • Astronomy & Astrophysics
  • FORMATION LAW
  • FORMATION RATES
  • II.
  • MASS
  • MOLECULAR GAS
  • NEARBY GALAXIES
  • Physical Sciences
  • Science & Technology
  • galaxies: ISM
  • galaxies: evolution
  • galaxies: general
  • galaxies: star formation

Digital Object Identifier (DOI)

publisher

  • OXFORD UNIV PRESS

start page

  • L39

end page

  • L43

volume

  • 493

issue

  • 1