Dusty ring nebulae around new candidate Luminous Blue Variables

Astronomy and Astrophysics

Volumn 412, Issue 1, 2003, Pages 185-198

  Clark, J S ^a   Egan, M P ^b   Crowther, P A ^a,g   Mizuno, D R ^c   Larionov, V M ^d,e   Arkharov, A ^f  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b AIR FORCE RESEARCH LABORATORY   (United States)

^c BOSTON COLLEGE   (United States)

^d ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

^e Isaac Newton Institute of Chile   (Russian Federation)

^f RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

^g UNIVERSITY OF SHEFFIELD   (United Kingdom)

Author keywords

Stars: circumstellar matter; Stars: emission line, Be; Stars: winds, outflows

Indexed keywords

DUST; HELIUM; HYDROGEN; IMAGE ANALYSIS; INFRARED IMAGING; INFRARED SPECTROSCOPY; SIGNAL TO NOISE RATIO; SOLAR SYSTEM; WIND EFFECTS;

LUMINOUS BLUE VARIABLES (LBV); STARS;

ASTROPHYSICS;

EID: 0346332769     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031372     Document Type: Review

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