On the Formation of the Most Massive Stars in the Galaxy

The 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 thesis presents results of Submillimeter Array (SMA) and Very L...

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Bibliographic Details
Main Author: Galván-Madrid, Roberto J. (Author)
Corporate Author: SpringerLink (Online service)
Format: Electronic eBook
Language:English
Published: New York, NY : Springer New York : Imprint: Springer, 2012.
Series:Springer Theses, Recognizing Outstanding Ph.D. Research,
Subjects:
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ΒΚΠ - Πατρα: ALFd

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ΒΚΠ - Πατρα: BSC

Holdings details from ΒΚΠ - Πατρα: BSC
Call Number: 330.01 BAU
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