Photometry of the Rubin Losee blue stars at the anticenter

Details Photometry of the Rubin Losee blue stars at the anticenter Photometry of the Rubin Losee blue stars at the anticenter

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102..654p&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, June 1990, p. 654-657.

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2

B Stars, Blue Stars, Stellar Spectrophotometry, Interstellar Extinction, Milky Way Galaxy, Stellar Luminosity, Ubv Spectra

Scientific paper

The present UBV and uvby observations of 14 Rubin and Losee (1971) stars in the anticenter region of the Galaxy confirm these stars' classification as normal, Population I B stars. These judgments have their basis in computations for each star of intrinsic colors, implied spectral types, and interstellar reddenings in both systems. Reasonable photometric distance estimates place some of these stars at large distances from the sun, estimated to be of up to 10 kpc.

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