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Galván-Madrid, Roberto J.
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This thesis presents results of Submillimeter Array (SMA) and Very Large Array (VLA) studies of massive star formation regions in the early stages of ionization, as well as an analysis of numerical simulations of the evolution of these young HII regions. The results favor a picture in which very massive stars form in accretion flows that are partially ionized and that keep accreting material from their environment ...
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New York: [Springer, ], 2012
e20424989
eBooks Universitas Indonesia Library