Study of candidate Be stars in the Magellanic Clouds using near-infrared photometry and optical spectroscopy

Monthly Notices of the Royal Astronomical Society

Volumn 421, Issue 4, 2012, Pages 3622-3640

  Paul, K T ^a   Subramaniam, A ^b   Mathew, B ^b,c   Mennickent, R E ^d   Sabogal, B ^e  

^a CHRIST DEEMED TO BE UNIVERSITY   (India)

^b INDIAN INSTITUTE OF ASTROPHYSICS   (India)

^c PHYSICAL RESEARCH LABORATORY   (India)

^d UNIVERSITY OF CONCEPCIÓN   (Chile)

^e UNIVERSIDAD DE LOS ANDES   (Colombia)

Author keywords

Circumstellar matter; Magellanic Clouds; Stars: emission line, Be; Techniques: spectroscopic

Indexed keywords

EID: 84859595749     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2012.20591.x     Document Type: Article

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