Formation and evolution of planetary systems: properties of debris dust around solar-type stars

Astrophysical Journal, Supplement Series

Volumn 181, Issue 1, 2009, Pages 197-226

  Carpenter, John M ^a   Jeroen, Bouwman ^b   Mamajek, Eric E ^c   Meyer, Michael R ^d   Hillenbrand, Lynne A ^a   Backman, Dana E ^e   Thomas, Henning ^b   Hines, Dean C ^f   David, Hollenbach ^g   Jinyoung, Serena Kim ^d   Amaya, Moro Martin ^h   Ilaria, Pascucci ^d   Silverstone, Murray D ⁱ   Stauffer, John R ^j   Sebastian, Wolf ^b  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c UNIVERSITY OF ROCHESTER   (United States)

^d UNIVERSITY OF ARIZONA   (United States)

^e SETI INSTITUTE   (United States)

^f Center for Extrasolar Planetary Systems   (United States)

^g NASA AMES RESEARCH CENTER   (United States)

^h PRINCETON UNIVERSITY   (United States)

ⁱ Eureka Scientific Inc   (United States)

^j CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

more..

Author keywords

Circumstellar matter; Infrared: Stars; Planetary systems: Formation

Indexed keywords

EID: 66649115237     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1088/0067-0049/181/1/197     Document Type: Article

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