The spectral energy distribution and mass-loss history of IRC + 10420

Monthly Notices of the Royal Astronomical Society

Volumn 280, Issue 4, 1996, Pages 1062-1070

  Oudmaijer, René D ^a,b   Groenewegen, M A T ^c   Matthews, H E ^d,e   Blommaert, J A D L ^f,h   Sahu, K C ^g  

^a UNIVERSITY OF GRONINGEN   (Netherlands)

^b IMPERIAL COLLEGE LONDON   (United Kingdom)

^c Werner Heisenberg Institut für Physik   (Germany)

^d UNIVERSITY OF HAWAII   (United States)

^e NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^f CNRS   (France)

^g STScI   (United States)

^h ISO Science Operations Centre   (Spain)

Author keywords

Circumstellar matter; Stars: AGB and post AGB; Stars: evolution; Stars: individual: IRC + 10420; Stars: mass loss; Supergiants

Indexed keywords

PHOTOMETRY; RADIATIVE TRANSFER; STARS;

CIRCUMSTELLAR MATTERS; DISTRIBUTION LOSS; HOT COMPONENTS; SPECTRAL ENERGY DISTRIBUTION; STAR: EVOLUTION; STAR: INDIVIDUAL: IRC + 10420; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MASS-LOSS; STARS:AGB AND POST AGB; SUPERGIANT;

SPECTROSCOPY;

EID: 1542505615     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/280.4.1062     Document Type: Article

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