Mid-ultraviolet and optical photometry of helium stars

Details Mid-ultraviolet and optical photometry of helium stars Mid-ultraviolet and optical photometry of helium stars

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992japa...13..175k&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 13, no. 2, June 1992, p. 175-194.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, B Stars, Stellar Atmospheres, Stellar Spectra, Stellar Temperature, Ultraviolet Astronomy, Helium, Radiant Flux Density, Ultraviolet Spectra

Scientific paper

Mid-ultraviolet and optical photometric analysis of helium stars are
presented. A linear relation exists between the effective temperature
derived from model atmospheres and (1965-V)0 index. The effective
temperatures derived from (1965-V)0 index are somewhat higher than that
of MK spectral type estimates especially for late B-type helium objects.

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