Titlebook: On the Formation of the Most Massive Stars in the Galaxy; Roberto J. Galván-Madrid Book 2012 Springer Science+Business Media New York 2012

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愛花花兒憤怒

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2190-5053 nization.Author has received the 2010 Doxey Prize, given outThe most massive stars in the galaxy - those with more than 15 to 20 solar masses - are lilkely to ionize their surroundings before they reach their final mass. How can they accrete in spite of the presence of over-pressurized gas? .This th

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Book 2012evolution 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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Book 2012inal mass. How can they accrete in spite of the presence of over-pressurized gas? .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

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A MSFR with Young UC and HC HII Regions: G20.08N,Spectral line and continuum observations of the molecular and ionized gas in G20.08–0.14N explore the dynamics over a range of spatial scales in this massive star-forming region.

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Conclusions,In this thesis we have performed radio to (sub)mm observations (Chaps. 2 and 3) in continuum, molecular lines, and hydrogen recombination lines that reveal the structure and dynamics of two MSFRs with very high luminosities (. > 10...) that are in the process of forming stars at the upper end of the mass function.

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978-1-4614-3307-1Springer Science+Business Media New York 2012