The distance to the large magellanic cloud cluster reticulum from the K-band period-luminosity-metallicity relation of RR lyrae stars

Astrophysical Journal

Volumn 610, Issue 1 I, 2004, Pages 269-274

  Dall'Ora, M ^a   Storm, J ^b   Bono, G ^a   Ripepi, V ^c   Monelli, M ^a   Testa, V ^a   Andreuzzi, G ^a,d   Buonanno, R ^e   Caputo, F ^a   Castellani, V ^a   Corsi, C E ^a   Marconi, G ^f   Marconi, M ^c   Pulone, L ^a   Stetson, P B ^g  

^a INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^b ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^c INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

^d FUNDACIÓN GALILEO GALILEI INAF   (Spain)

^e UNIVERSITY OF ROME TOR VERGATA   (Italy)

^f EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^g NATIONAL RESEARCH COUNCIL CANADA   (Canada)

Author keywords

Stars: evolution; Stars: oscillations; Stars: variables: other

Indexed keywords

EID: 4444226949     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/421513     Document Type: Article

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