The state of protoplanetary material 10 million years after stellar formation: Circumstellar disks in the TW hydrae association

Astrophysical Journal, Supplement Series

Volumn 154, Issue 1, 2004, Pages 439-442

  Uchida, K I ^a   Calvet, N ^b   Hartmann, L ^b   Kemper, F ^c   Forrest, W J ^d   Watson, D M ^d   D'Alessio, P ^e   Chen, C H ^f   Furlan, E ^a   Sargent, B ^d   Brandl, B R ^g   Herter, T L ^a   Morris, P ^h   Myers, P C ^b   Najita, J ⁱ   Sloan, G C ^a   Barry, D J ^a   Green, J ^d   Keller, L D ^j   Hall, P ^a  

^a Department of Astronomy and Center for Radiophysics and Space Research   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d UNIVERSITY OF ROCHESTER   (United States)

^e CENTRO DE RADIOASTRONOMÍA Y ASTROFÍSICA   (Mexico)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g LEIDEN UNIVERSITY   (Netherlands)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^j ITHACA COLLEGE   (United States)

more..

Author keywords

Accretion, accretion disks; Circumstellar matter; Infrared: stars; Stars: formation; Stars: pre main sequence

Indexed keywords

EID: 5644269318     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/422888     Document Type: Article

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