New insights into the nature of the SMC WR/LBV binary HD 5980

Revista Mexicana de Astronomia y Astrofisica

Volumn 44, Issue 1, 2008, Pages 3-27

  Foellmi, C ^a   Koenigsberger, G ^b   Georgiev, L ^c   Toledano, O ^b   Marchenko, S V ^d   Massey, P ^e,f   Dall, T H ^f   Moffat, A F J ^g,q   Morrell, N ^h   Corcoran, M ^i,j,o   Kaufer, A ^k   Naze Y ^l   Pittard, J ^m   St Louis, N ^g,q   Fullerton, A ⁿ   Massa, D ^o   Pollock, A M T ^p  

^a LABORATOIRE D ASTROPHYSIQUE   (France)

^b INSTITUTO DE CIENCIAS FÍSICAS   (Mexico)

^c UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^d WESTERN KENTUCKY UNIVERSITY   (United States)

^e LOWELL OBSERVATORY   (United States)

^f GEMINI OBSERVATORY   (United States)

^g UNIVERSITÉ DE MONTRÉAL   (Canada)

^h LAS CAMPANAS OBSERVATORY   (Chile)

ⁱ X ray Astrophysics Laboratory NASA/ GSFC   (United States)

^j UNIVERSITIES SPACE RESEARCH ASSOCIATION   (United States)

^k EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^l UNIVERSITY OF LIÈGE   (Belgium)

^m UNIVERSITY OF LEEDS   (United Kingdom)

ⁿ STScI   (United States)

^o NASA GODDARD SPACE FLIGHT CENTER   (United States)

^p EUROPEAN SPACE AGENCY   (Spain)

^q Observatoire du Mont Mégamtic   (Canada)

more..

Author keywords

Binaries: close; Stars: individual (HD 5980); Stars: mass loss

Indexed keywords

EID: 42449149126     PISSN: 01851101     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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