Identification of main-sequence stars with mid-infrared excesses using glimpse: β pictoris analogs?

Astrophysical Journal

Volumn 629, Issue 1 I, 2005, Pages 512-525

  Uzpen, B ^a   Kobulnicky, H A ^a   Olsen, K A G ^b   Clemens, D P ^c   Laurance, T L ^a   Meade, M R ^d   Babler, B L ^d   Indebetouw, R ^d   Whitney, B A ^e   Watson, C ^d   Wolfire, M G ^f   Wolff, M J ^e   Benjamin, R A ^g   Bania, T M ^c   Cohen, M ^h   Devine, K E ^d   Dickey, J M ⁱ   Heitsch, F ^j   Jackson, J M ^c   Marston, A P ^k   Mathis, J S ^d   Mercer, E P ^c   Stauffer, J R ^l   Stolovy, S R ^l   Backman, D E ^m   Churchwell, E ^d   more..

^a UNIVERSITY OF WYOMING   (United States)

^b CERRO TOLOLO INTER AMERICAN OBSERVATORY   (Chile)

^c BOSTON UNIVERSITY   (United States)

^d UNIVERSITY OF WISCONSIN MADISON   (United States)

^e Center for Extrasolar Planetary Systems   (United States)

^f Bldg 142   (United States)

^g UNIVERSITY OF WISCONSIN WHITEWATER   (United States)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ University of Minnesota   (United States)

^j UNIVERSITY OF MUNICH   (Germany)

^k EUROPEAN SPACE AGENCY   (Netherlands)

^l CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^m NASA AMES RESEARCH CENTER   (United States)

more..

Author keywords

Circumstellar matter; Open clusters and associations: individual (Westerlund 2); Planetary systems: formation

Indexed keywords

EID: 28144442602     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/431479     Document Type: Article

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