Other
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aj.....90.1464s&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 90, Aug. 1985, p. 1464-1473.
Other
74
Cepheid Variables, Color-Magnitude Diagram, Dwarf Galaxies, Reference Stars, Stellar Magnitude, Stellar Spectrophotometry, Supergiant Stars, Blue Stars, Calibrating, Electrophotometry, Light Curve, Red Giant Stars, Stellar Evolution
Scientific paper
The brightest red and blue supergiants in the nearby, highly resolved Im IV-V galaxy WLM have been identified and photometered relative to a photoelectric sequence measured to V = 18.6, B = 19.5. The sequence is extended to V = 22, B = 23. The mean magnitudes for the three brightest blue and red supergiants are = 17.74 (or 17.69 depending on membership) for the blue stars, and
Carlson Glenn
Sandage Alan
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