Properties of galactic B[e] supergiants: III. MWC 300

Astronomy and Astrophysics

Volumn 417, Issue 2, 2004, Pages 731-743

  Miroshnichenko, A S ^a,b   Levato, H ^c   Bjorkman, K S ^a   Grosso, M ^c   Manset, N ^d   Men'shchikov, A B ^e,f   Rudy, R J ^g   Lynch, D K ^g   Mazuk, S ^g   Venturini, C C ^g   Puetter, R C ^h   Perry, R B ⁱ  

^a UNIVERSITY OF TOLEDO   (United States)

^b RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

^c Complejo Astron El Leoncito ^*  (Argentina)

^d CANADA FRANCE HAWAII TELESCOPE   (United States)

^e MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^f SAINT MARY S UNIVERSITY   (Canada)

^g AEROSPACE CORPORATION   (United States)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ NASA LANGLEY RESEARCH CENTER   (United States)

Author keywords

Circumstellar matter radiative transfer; Stars: emission line, Be; Stars: individual: MWC 300; Techniques: spectroscopic

Indexed keywords

ABSORPTION; HELIUM; INFRARED IMAGING; ORBITS; PHOTOMETRY; SIGNAL TO NOISE RATIO; SOLAR RADIATION; SPECTROGRAPHS; SPECTROSCOPY;

CIRCUMSTELLAR MATTER; RADIATIVE TRANSFER; STARS:EMISSION-LINE, BE; STARS:INDIVIDUAL:MWC 300; TECHNIQUES:SPECTROSCOPIC;

GALAXIES;

EID: 11144357443     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034181     Document Type: Article

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