How do central and satellite galaxies quench? - Insights from spatially resolved spectroscopy in the MaNGA survey Article

Bluck, Asa FL, Maiolino, Roberto, Piotrowska, Joanna M et al. (2020). How do central and satellite galaxies quench? - Insights from spatially resolved spectroscopy in the MaNGA survey . MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 499(1), 230-268. 10.1093/mnras/staa2806

Open Access International Collaboration

cited authors

  • Bluck, Asa FL; Maiolino, Roberto; Piotrowska, Joanna M; Trussler, James; Ellison, Sara L; Sanchez, Sebastian F; Thorp, Mallory D; Teimoorinia, Hossen; Moreno, Jorge; Conselice, Christopher J

authors

publication date

  • November 1, 2020

keywords

  • ACTIVE GALACTIC NUCLEI
  • AGN FEEDBACK
  • Astronomy & Astrophysics
  • COOLING FLOWS
  • FUNDAMENTAL RELATION
  • Galaxy: bulge
  • Galaxy: disc
  • LOCAL UNIVERSE
  • PHOTOMETRIC PROPERTIES
  • Physical Sciences
  • SDSS-IV MANGA
  • STAR-FORMING GALAXIES
  • STELLAR MASS
  • SUPERMASSIVE BLACK-HOLES
  • Science & Technology
  • galaxies: evolution
  • galaxies: formation
  • galaxies: star formation
  • galaxies: statistics

Digital Object Identifier (DOI)

publisher

  • OXFORD UNIV PRESS

start page

  • 230

end page

  • 268

volume

  • 499

issue

  • 1