The MACHO project large magellanic cloud variable star inventory. XI. Frequency analysis of the fundamental-mode RR Lyrae stars

Astrophysical Journal

Volumn 598, Issue 1 I, 2003, Pages 597-609

  Alcock, C ^a,b,c   Alves, D R ^d   Becker, A ^e   Bennett, D ^b,f   Cook, K H ^b,c   Drake, A ^b,g   Freeman, K ^h   Geha, M ⁱ   Griest, K ^j   Kovacs G ^k   Lehner, M ^a   Marshall, S ^b   Minniti, D ^g   Nelson, C ^b,c   Peterson, B ^h   Popowski, P ^l   Pratt, M ^m   Quinn, P ⁿ   Rodgers, A ^q   Stubbs, C ^c,m   Sutherland, W ^o   Vandehei, T ^j   Welch, D L ^p   more..

^a UNIVERSITY OF PENNSYLVANIA   (United States)

^b LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d Mail Code 5247 ^*  (United States)

^e LUCENT TECHNOLOGIES   (United States)

^f UNIVERSITY OF NOTRE DAME   (United States)

^g PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^h AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

^j UNIVERSITY OF CALIFORNIA   (United States)

^k KONKOLY OBSERVATORY   (Hungary)

^l MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^m UNIVERSITY OF WASHINGTON   (United States)

ⁿ EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^o UNIVERSITY OF OXFORD   (United Kingdom)

^p MCMASTER UNIVERSITY   (Canada)

^q NONE

more..

Author keywords

Globular clusters: general; Stars: horizontal branch; Stars: oscillations; Stars: variables: other (RR Lyrae)

Indexed keywords

EID: 0348156866     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/378689     Document Type: Article

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