Tomographic separation of composite spectra. VII. The physical properties of the massive triple system HD 135240 (δ circini)

Astrophysical Journal

Volumn 548, Issue 2 PART 1, 2001, Pages 889-899

  Penny, Laura R ^a   Seyle, Debra ^a   Gies, Douglas R ^b   Harvin, James A ^b   Bagnuolo Jr , William G ^b   Thaller, M L ^c   Fullerton, A W ^d,f   Kaper, L ^e  

^a School of Business and Economics   (United States)

^b GEORGIA STATE UNIVERSITY   (United States)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d UNIVERSITY OF VICTORIA   (Canada)

^e UNIVERSITY OF AMSTERDAM   (Netherlands)

^f JOHNS HOPKINS UNIVERSITY   (United States)

Author keywords

Binaries: eclipsing; Binaries: spectroscopic; Stars: early type; Stars: fundamental parameters; Stars: individual (HD 135240); Ultraviolet: stars

Indexed keywords

EID: 0035916444     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/319031     Document Type: Article

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