On the nature of the high-latitude B-type star CPD-61°455

Monthly Notices of the Royal Astronomical Society

Volumn 278, Issue 3, 1996, Pages 811-820

  Hambly, N C ^a,c   Dufton, P L ^a   Keenan, F P ^a   Lumsden, S L ^b  

^a QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^b ANGLO AUSTRALIAN OBSERVATORY   (Australia)

^c UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

Author keywords

Binaries: general; Infrared: stars; Stars: AGB and post AGB; Stars: early type; Stars: individual: CPD 61 455

Indexed keywords

LIGHT ABSORPTION; NEAR INFRARED SPECTROSCOPY; SIGNAL TO NOISE RATIO; STARS; SYSTEMS (METALLURGICAL);

ASYMPTOTIC GIANT BRANCH; BINARIES:GENERAL; HIGH LATITUDES; INFRARED: STAR; OPTICAL-; STAR: AGB AND POST-ASYMPTOTIC GIANT BRANCH; STAR: INDIVIDUAL: CPD-61°455; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:AGB; STARS:EARLY TYPE;

INFRARED DEVICES;

EID: 0012962418     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/278.3.811     Document Type: Article

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