Formation and evolution of planetary systems: Upper limits to the gas mass in disks around sun-like stars

Astrophysical Journal

Volumn 651, Issue 2 I, 2006, Pages 1177-1193

  Pascucci, I ^a   Gorti, U ^b   Hollenbach, D ^c   Najita, J ^d   Meyer, M R ^a   Carpenter, J M ^e   Hillenbrand, L A ^e   Herczeg, G J ^e   Padgett, D L ^e   Mamajek, E E ^f   Silverstone, M D ^a   Schlingman, W M ^a   Kim, J S ^a   Stobie, E B ^a   Bouwman, J ^g   Wolf, S ^g   Rodmann, J ^g   Hines, D C ^h   Lunine, J ^a   Malhotra, R ^a  

^a UNIVERSITY OF ARIZONA   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c NASA AMES RESEARCH CENTER   (United States)

^d NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^g MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^h Center for Extrasolar Planetary Systems   (United States)

Author keywords

Circumstellar matter; Infrared: stars; Planetary systems: formation; Solar system: formation

Indexed keywords

EID: 33845746232     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/507761     Document Type: Article

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