The MACHO project Large Magellanic Cloud variable-star inventory. IX. Frequency analysis of the first-overtone RR Lyrae stars and the indication for nonradial pulsations

Astrophysical Journal

Volumn 542, Issue 1 PART 1, 2000, Pages 257-280

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

^a LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^b AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^c AURA for the European Space Agency   (United States)

^d UNIVERSITY OF WASHINGTON   (United States)

^e UNIVERSITY OF NOTRE DAME   (United States)

^f UNIVERSITY OF TORONTO   (Canada)

^g UNIVERSITY OF CALIFORNIA   (United States)

^h KONKOLY OBSERVATORY   (Hungary)

ⁱ UNIVERSITY OF CAPE TOWN   (South Africa)

^j UNIVERSITY OF CALIFORNIA   (United States)

^k EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^l MCMASTER UNIVERSITY   (Canada)

^m NONE

more..

Author keywords

Globular clusters: general; Magellanic clouds; Stars: horizontal branch; Stars: oscillations; Stars: variables: other

Indexed keywords

EID: 0034633428     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/309530     Document Type: Article

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