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- W186738144 abstract "We are studying how precise astrometric measurements by SIM of the nearest young massive stars can constrain their dynamical history. In the particular case of 1Ori C, this constrains the properties of a recent dynamical ejection event, which is influencing the Orion KL massive protostar. We are also searching for lower mass candidate runaway stars from the ONC with Hipparcos data. Follow up with SIM can confirm their runaway nature and constrain the formation history of the cluster. Star clusters, like the Orion Nebula Cluster (ONC) pictured right in a JHK image, are the sites of most star formation and essentially all massive star formation (Lada & Lada 2003; de Wit et al. 2005). Orion KL massive protostar" @default.
- W186738144 created "2016-06-24" @default.
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- W186738144 date "2009-01-01" @default.
- W186738144 modified "2023-10-16" @default.
- W186738144 title "Stellar Dynamical Processes in Massive Star and Star Cluster Formation" @default.
- W186738144 hasPublicationYear "2009" @default.
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