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astro-ph.SRFeb 1, 2017
2
citations (OpenAlex)
authors
  • Philip Massey
  • Emily Levesque
  • Kathryn Neugent
  • Kate Evans
  • Maria Drout
  • Madeleine Beck
institutions
  • California Institute of Technology
  • Carnegie Institution for Science
  • Carnegie Observatories
  • Lowell Observatory
  • Northern Arizona University
  • University of Washington
  • Wellesley College
arXiv abstractPDF
paper

The Red Supergiant Content of the Local Group

arXiv:1702.00221 · doi:10.1017/S1743921317002642

Abstract

We summarize here recent work in identifying and characterizing red supergiants (RSGs) in the galaxies of the Local Group.

To appear in IAU 329, The Lives and Death-throes of Massive Stars, ed. J. J. Eldridge

References in corpus (8)

  • Binary interaction dominates the evolution of massive stars
  • BPASS predictions for Binary Black-Hole Mergers
  • The Effective Temperatures and Physical Properties of Magellanic Cloud Red Supergiants: The Effects of Metallicity
  • Late-Type Red Supergiants: Too Cool for the Magellanic Clouds?
  • Discovery of a Thorne-Zytkow object candidate in the Small Magellanic Cloud
  • The Red Supergiant Content of M31
  • Large proper motion of the Thorne-Żytkow object candidate HV 2112 reveals its likely nature as foreground Galactic S-star
  • The proper motion of HV2112: A TŻO candidate in the SMC

Cited by in corpus (1)

  • The Masses of Supernova Remnant Progenitors in M33
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