The (sub-)millimeter SED of protoplanetary disks in the outskirts of the Orion nebula cluster

Astronomy and Astrophysics

Volumn 525, Issue 19, 2011, Pages

  Ricci, L ^a   Mann, R K ^b   Testi, L ^a   Williams, J P ^c   Isella, A ^d   Robberto, M ^e   Natta, A ^f   Brooks, K J ^g  

^a EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^b NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^c UNIVERSITY OF HAWAII   (United States)

^d California Institute of Technology   (United States)

^e STScI   (United States)

^f INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^g CSIRO   (Australia)

Author keywords

Planets and satellites: formation; Protoplanetary disks; Stars: pre main sequence

Indexed keywords

CIRCUMSTELLAR DISKS; CLUSTER CENTERS; HIGH-MASS STARS; LOW-MASS STARS; ORION NEBULA; PLANETS AND SATELLITES: FORMATION; PROTOPLANETARY DISKS; SPECTRAL INDICES; STARS: PRE-MAIN SEQUENCE; SUBMILLIMETER WAVELENGTHS;

DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); DUST; GRAIN SIZE AND SHAPE; PLANETS; SATELLITES; STARS;

GRAIN GROWTH;

EID: 79951500696     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: None     Document Type: Article

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