HUBBLE SPACE TELESCOPE MEASURES OF MASS ACCRETION RATES IN THE ORION NEBULA CLUSTER

The present observational understanding of the evolution of the mass accretion rates ([dot over M][subscript acc]) in pre-main-sequence stars is limited by the lack of accurate measurements of [dot over M][subscript acc] over homogeneous and large statistical samples of young stars. Such observation...

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Bibliographic Details
Main Authors: Manara, C. F. (Author), Robberto, M. (Author), Da Rio, N. (Author), Lodato, G. (Author), Hillenbrand, L. A. (Author), Soderblom, D. R. (Author), Stassun, Keivan (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-02-25T13:45:57Z.
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