The MACHO project Large Magellanic Cloud variable star inventory. III. Multimode RR Lyrae stars, distance to the Large Magellanic Cloud, and age of the oldest stars

Astrophysical Journal

Volumn 482, Issue 1 PART I, 1997, Pages 89-97

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

^a LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^d AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^e UNIVERSITY OF WASHINGTON   (United States)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g UNIVERSITY OF CALIFORNIA   (United States)

^h EUROPEAN SOUTHERN OBSERVATORY   (Germany)

ⁱ UNIVERSITY OF OXFORD   (United Kingdom)

^j MCMASTER UNIVERSITY   (Canada)

more..

Author keywords

Galaxies: distances and redshifts; Magellanic Clouds; Stars: oscillations; Stars: variables: other (RR Lyrae)

Indexed keywords

EID: 21744438183     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/304120     Document Type: Article

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