4.6 Article

THE MASSIVE STAR POPULATION IN M101. III. SPECTRA AND PHOTOMETRY OF THE LUMINOUS AND VARIABLE STARS

期刊

ASTRONOMICAL JOURNAL
卷 149, 期 5, 页码 -

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IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/149/5/152

关键词

galaxies: individual (M101); supergiants

资金

  1. National Science Foundation [AST-1109394]
  2. Division Of Astronomical Sciences
  3. Direct For Mathematical & Physical Scien [1109394] Funding Source: National Science Foundation

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We discuss moderate-resolution spectra, multicolor photometry, and light curves of 31 of the most luminous stars and variables in the giant spiral M101. The majority are intermediate A-to F-type supergiants. We present new photometry and light curves for three known irregular blue variables, V2, V4, and V9, and identify a new candidate. Their spectra and variability confirm that they are luminous blue variable (LBV) candidates and V9 may be in an LBV-like maximum light state or eruption.

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