Ultraviolet spectrophotometry of variable early-type be and B stars derived from high-resolution IUE data

Astrophysical Journal

Volumn 562, Issue 2 PART II, 2001, Pages 998-1011

  Smith, Myron A ^a,b  

^a STScI   (United States)

^b CATHOLIC UNIVERSITY OF AMERICA   (United States)

Author keywords

Circumstellar matter; Stars: emission line, be; Stars: oscillations; Ultraviolet: stars

Indexed keywords

EID: 0141901826     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/323846     Document Type: Article

References (5)

1. Baade, D. 2000, in ASP Conf. Ser. 214, The Be Phenomenon in Early-Type Stars, ed. M. A. Smith, H. F. Henrichs, & J. Fabregat (San Francisco: ASP), 178
2. Baade, D., & Balona, L. A. 1994, in Pulsation, Rotation, & Mass Loss in Early-Type stars, ed. L. Balona, H. Henrichs, & J. Le Contel (Dordrecht: Kluwer), 311
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