Galactic clusters with associated Cepheid variables - VII. Berkeley 58 and CG Cassiopeiae

Monthly Notices of the Royal Astronomical Society

Volumn 388, Issue 1, 2008, Pages 444-456

  Turner, D G ^a   Forbes, D ^b   English, D ^b   Leonard, P J T ^c   Scrimger, J N ^d   Wehlau, A W ^e   Phelps, R L ^f   Berdnikov, L N ^g   Pastukhova, E N ^h  

^a SAINT MARY S UNIVERSITY   (Canada)

^b MEMORIAL UNIVERSITY OF NEWFOUNDLAND   (Canada)

^c ADNET SYSTEMS INC   (United States)

^d DALHOUSIE UNIVERSITY   (Canada)

^e UNIVERSITY OF WESTERN ONTARIO   (Canada)

^f Division of Astronomical Sciences   (United States)

^g MOSCOW STATE UNIVERSITY   (Russian Federation)

^h INSTITUTE OF ASTRONOMY   (Russian Federation)

Author keywords

Cepheids; Open clusters and associations: individual: Berkeley 58; Stars: evolution

Indexed keywords

ASTROPHYSICS;

CEPHEIDS; EARLY-TYPE - STARS; LIGHT AMPLITUDE; OPEN CLUSTER AND ASSOCIATION: INDIVIDUAL: BERKELEY 58; OPEN CLUSTERS; OPEN CLUSTERS AND ASSOCIATION: INDIVIDUAL; PHOTOELECTRICS; RADIAL VELOCITY; SPIRAL ARMS; STAR: EVOLUTION;

STARS;

EID: 62349117600     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13413.x     Document Type: Article

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