Spectral energy distributions of passive T Tauri and Herbig Ae disks: Grain mineralogy, parameter dependences, and comparison with infrared space observatory LWS observations

Astrophysical Journal

Volumn 547, Issue 2 PART 1, 2001, Pages 1077-1089

  Chiang, E I ^a,b   Joung, M K ^b,c   Criech Eakman, M J ^d,e   Qi, C ^e   Kessler, J E ^f   Blake, G A ^e,f   Van Dishoeck, E F ^g  

^a INSTITUTE FOR ADVANCED STUDY   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c Och Spine at New York Presbyterian Hospitals   (United States)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f California Institute of Technology   (United States)

^g LEIDEN UNIVERSITY   (Netherlands)

Author keywords

Accretion, accretion disks; Circumstellar matter; Radiative transfer; Stars: individual (MWC 480, HD 36112, CQ Tauri, LkCa 15, AA Tauri); Stars: pre main sequence

Indexed keywords

EID: 0035255449     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/318427     Document Type: Article

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