Spectral energy distribution modelling of southern candidate massive protostars using the Bayesian inference method

Monthly Notices of the Royal Astronomical Society

Volumn 392, Issue 2, 2009, Pages 768-782

  Hill, T ^a,b,c   Pinte, C ^a   Minier, V ^d   Burton, M G ^c   Cunningham, M R ^c  

^a UNIVERSITY OF EXETER   (United Kingdom)

^b LEIDEN UNIVERSITY   (Netherlands)

^c UNIVERSITY OF NEW SOUTH WALES   (Australia)

^d UNIVERSITÉ PARIS DIDEROT   (France)

Author keywords

H ii regions; Masers; Stars: early type; Stars: formation; Stars: fundamental parameters; Submillimetre

Indexed keywords

BAYESIAN NETWORKS; GIANT STARS; INFERENCE ENGINES; MASERS;

BAYESIAN INFERENCE; DISTRIBUTION MODELS; H II REGION; MASSIVE STARS; PROTOSTARS; SPECTRAL ENERGY DISTRIBUTION; STARS FORMATION; STARS:EARLY TYPE; STARS:FUNDAMENTAL PARAMETERS; SUBMILLIMETRE;

SPECTROSCOPY;

EID: 58049172289     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.14103.x     Document Type: Article

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