Interpreting spectral energy distributions from young stellar objects. II. Fitting observed SEDs using a large grid of precomputed models

Astrophysical Journal, Supplement Series

Volumn 169, Issue 2, 2007, Pages 328-352

  Robitaille, Thomas P ^a   Whitney, Barbara A ^b   Indebetouw, Remy ^c   Wood, Kenneth ^a  

^a UNIVERSITY OF ST ANDREWS   (United Kingdom)

^b Cassini Imaging Central Laboratory for Operations   (United States)

^c UNIVERSITY OF VIRGINIA   (United States)

Author keywords

Circumstellar matter; Infrared: stars; Radiative transfer; Stars: formation; Stars: pre main sequence

Indexed keywords

EID: 34248361157     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/512039     Document Type: Article

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