The late B-type stars: Refined MK classification, confrontation with stromgren photometry, and the effects of rotation

Details The late B-type stars: Refined MK classification, confrontation with stromgren photometry, and the effects of rotation The late B-type stars: Refined MK classification, confrontation with stromgren photometry, and the effects of rotation

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aj....107.1556g&link_type=abstract

The Astronomical Journal, vol. 107, no. 4, p. 1556-1564

Astronomy and Astrophysics

Astronomy

18

B Stars, F Stars, Photometry, Spectrum Analysis, Helium Isotopes, Iue, Luminosity, Spectral Sensitivity

Scientific paper

In the fourth and final of a series of papers on the late B to the early F type stars, we refine the Morgan Keenan (MK) spectral classification system for the late B type stars and consider the effect of rotation on both spectral classification and Stroemgren photometry of these stars. We extend the work of Morgan by establishing self-consistent sequences of narrow and broadlined standards. We reclassify a number of Bp stars, compare these classifications with Stroemgren photometry and consider the question of whether all Bp stars are main-sequence objects.

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