Formation and Evolution of Planetary Systems (FEPS): Primordial warm dust evolution from 3 to 30 Myr around Sun-like stars

Astrophysical Journal

Volumn 639, Issue 2 I, 2006, Pages 1138-1146

  Silverstone, M D ^a   Meyer, M R ^a   Mamajek, E E ^b   Hines, D C ^c   Hillenbrand, L A ^d   Najita, J ^e   Pascucci, I ^a   Bouwman, J ^f   Kim, J S ^a   Carpenter, J M ^d   Stauffer, J R ^g   Backman, D E ^h   Moro Martin, A ⁱ   Henning, T ^f   Wolf, S ^f   Brooke, T Y ^d   Padgett, D L ^g  

^a UNIVERSITY OF ARIZONA   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c Center for Extrasolar Planetary Systems   (United States)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^f MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^g CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^h NASA AMES RESEARCH CENTER   (United States)

ⁱ PRINCETON UNIVERSITY   (United States)

Author keywords

Infrared: stars; Planetary systems: protoplanetary disks; Stars: formation; Stars: pre main sequence

Indexed keywords

EID: 33645132826     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/499418     Document Type: Article

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