Tomographic separation of composite spectra. VIII. The physical properties of the massive compact binary in the triple star system HD 36486 (δ Orionis A)

Astrophysical Journal

Volumn 565, Issue 2 I, 2002, Pages 1216-1230

  Harvin, James A ^a   Gies, Douglas R ^a   Bagnuolo Jr , William G ^a   Penny, Laura R ^b   Thaller, Michelle L ^c,d  

^a GEORGIA STATE UNIVERSITY   (United States)

^b Department of Teacher Education and Department of Sociology and Anthropology   (United States)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

Author keywords

Binaries: eclipsing; Binaries: spectroscopic; Stars: early type; Stars: fundamental parameters; Stars: individual ( Orionis, HD 36486); Ultraviolet: stars

Indexed keywords

EID: 0010695619     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/324705     Document Type: Article

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