The MACHO project LMC variable star inventory. VI. The second overtone mode of cepheid pulsation from first/second overtone beat cepheids

Astrophysical Journal

Volumn 511, Issue 1 PART 1, 1999, Pages 185-192

  Alcock, C ^a,b   Allsman, R A ^c   Alves, D ^a,d   Axelrod, T S ^e   Becker, A C ^f   Bennett, D P ^a,b,g   Cook, K H ^a,b   Freeman, K C ^e   Griest, K ^b,h   Lehner, M J ^b,h,i   Marshall, S L ^a,b   Minniti, D ^a,b   Peterson, B A ^e   Pratt, M R ^b,f,j   Quinn, P J ^k   Rodgers, A W ^e   Rorabeck, A ^l   Sutherland, W ^m   Tomaney, A ^f   Vandehei, T ^b,h   Welch, D L ^l   more..

^a LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^f UNIVERSITY OF WASHINGTON   (United States)

^g UNIVERSITY OF NOTRE DAME   (United States)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ UNIVERSITY OF SHEFFIELD   (United Kingdom)

^j MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^k EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^l MCMASTER UNIVERSITY   (Canada)

^m UNIVERSITY OF OXFORD   (United Kingdom)

more..

Author keywords

Cepheids; Magellanic clouds; Stars: Fundamental parameters; Stars: Oscillations

Indexed keywords

EID: 0033585316     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/306638     Document Type: Article

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