The ultraviolet reddening of Be stars

Details The ultraviolet reddening of Be stars The ultraviolet reddening of Be stars

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...120..223s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 120, no. 2, April 1983, p. 223-226.

Astronomy and Astrophysics

Astrophysics

13

B Stars, Interstellar Extinction, Stellar Color, Ultraviolet Radiation, Energy Distribution, Star Clusters, Stellar Envelopes, Stellar Luminosity, Stellar Motions

Scientific paper

The UV extinction of several bright Be stars is examined in light of Schild's (1978) demonstration of their intrinsic (B-V) color excess. Stars possessing this excess are found not to have the 0.22-micron bump associated with Bless and Savage's (1972) interstellar reddening law. The bright Be stars studied are HD 30076, HD 58011, HD 63462, and HD 105435.

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