New debris disks around nearby main-sequence stars: Impact on the direct detection of planets

Astrophysical Journal

Volumn 652, Issue 2 I, 2006, Pages 1674-1693

  Beichman, C A ^a   Bryden, G ^b   Stapelfeldt, K R ^b   Gautier, T N ^b   Grogan, K ^b   Shao, M ^b   Velusamy, T ^b   Lawler, S M ^a   Blaylock, M ^c   Rieke, G H ^c   Lunine, J I ^c   Fischer, D A ^d   Marcy, G W ^e   Greaves, J S ^f   Wyatt, M C ^g   Holland, W S ^h   Dent, W R F ^h  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c UNIVERSITY OF ARIZONA   (United States)

^d SAN FRANCISCO STATE UNIVERSITY   (United States)

^e UNIVERSITY OF CALIFORNIA   (United States)

^f UNIVERSITY OF ST ANDREWS   (United Kingdom)

^g UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^h UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

Author keywords

Circumstellar matter; Infrared: stars; Kuiper belt

Indexed keywords

EID: 33845887751     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/508449     Document Type: Article

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