HST images do not support the presence of three high-velocity, low-mass runaway stars in the core of the Orion Nebula cluster

Astrophysical Journal

Volumn 633, Issue 1 II, 2005, Pages

  O'Dell, C R ^a   Poveda, Arcadio ^b   Allen, Christine ^b   Robberto, Massimo ^c  

^a VANDERBILT UNIVERSITY   (United States)

^b UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^c STScI   (United States)

Author keywords

Astrometry; Stars: kinematics; Stars: pre main sequence

Indexed keywords

EID: 29144527504     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/498450     Document Type: Article

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