Spectroscopic study of the long-period dust-producing WC7pd+O9 binary HD 192641

Monthly Notices of the Royal Astronomical Society

Volumn 360, Issue 1, 2005, Pages 141-152

  Lefevre L ^a,b   Marchenko, S V ^c   Lepine S ^d   Moffat, A F J ^a   Acker, A ^b   Harries, T J ^e   Annuk, K ^f   Bohlender, D A ^g   Demers, H ^a   Grosdidier, Y ^h   Hill, G M ⁱ   Morrison, N D ^j   Knauth, D C ^k   Skalkowski, G ^a   Viti, S ^l  

^a UNIVERSITÉ DE MONTRÉAL   (Canada)

^b OBSERVATOIRE DE STRASBOURG   (France)

^c WESTERN KENTUCKY UNIVERSITY   (United States)

^d DIVISION OF INVERTEBRATE ZOOLOGY   (United States)

^e UNIVERSITY OF EXETER   (United Kingdom)

^f TARTU OBSERVATORY   (Estonia)

^g NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^h MCGILL UNIVERSITY   (Canada)

ⁱ W M KECK OBSERVATORY   (United States)

^j UNIVERSITY OF TOLEDO   (United States)

^k NORTHWESTERN UNIVERSITY   (United States)

^l UNIVERSITY COLLEGE LONDON   (United Kingdom)

more..

Author keywords

Binaries: spectroscopic; Stars: oscillations; Stars: wind, outflows; Stars: Wolf Rayet

Indexed keywords

DUST; IONIZATION POTENTIAL; SPECTROSCOPIC ANALYSIS; STARS;

BINARIES: SPECTROSCOPIC; DATA COVER; EMISSION LINES; OPTICAL SPECTROSCOPIC STUDIES; SPECTROSCOPIC STUDIES; STAR OSCILLATIONS; STARS: WINDS OUTFLOWS; STARS: WOLF-RAYET; SUB-PEAKS;

ELECTROMAGNETIC WAVE EMISSION;

EID: 20744444566     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09017.x     Document Type: Article

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