CU COMAE: A new field double-mode RR Lyrae variable, the most metal-poor discovered to date

Astronomical Journal

Volumn 120, Issue 4, 2000, Pages 2054-2064

  Clementini, G ^a   Tomaso, S Di ^b   Fabrizio, L Di ^a   Bragaglia, A ^a   Merighi, R ^a   Tosi, M ^a   Carretta, E ^c   Gratton, R G ^c   Ivans, I I ^d   Kinard, A ^e   Marconi, M ^f   Smith, H A ^g   Wilhelm, R ^e   Woodruff, T ^e   Sneden, C ^d  

^a INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^b UNIVERSITY OF BOLOGNA   (Italy)

^c INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^d University of Texas at Austin   (United States)

^e SOUTHWESTERN UNIVERSITY   (United States)

^f INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

^g MICHIGAN STATE UNIVERSITY   (United States)

Author keywords

Abundances Stars; Fundamental parameters Stars; Horizontal branch stars; Individual (cu comae) Stars; Oscillations Stars; Other; Stars; Variables

Indexed keywords

EID: 0008607454     PISSN: 00046256     EISSN: None     Source Type: Journal    
DOI: 10.1086/301573     Document Type: Article

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