Evolution of mid-infrared excess around sun-like stars: Constraints on models of terrestrial planet formation

Astrophysical Journal

Volumn 673, Issue 2 PART 2, 2008, Pages

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

^a UNIVERSITY OF ARIZONA   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d NASA AMES RESEARCH CENTER   (United States)

^e PRINCETON UNIVERSITY   (United States)

^f NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^g Center for Extrasolar Planetary Systems   (United States)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^j SETI INSTITUTE   (United States)

more..

Author keywords

Circumstellar matter; Infrared: stars; Planetary systems: formation

Indexed keywords

EID: 67949107827     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/527470     Document Type: Article

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