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...
Published in: | Springer eBooks |
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Main Author: | Galván-Madrid, Roberto J. (Author) |
Corporate Author: | SpringerLink (Online service) |
Format: | eBook |
Language: | English |
Published: |
New York, NY :
Springer New York : Imprint: Springer,
2012.
|
Series: | Springer Theses, Recognizing Outstanding Ph.D. Research,
|
Subjects: | |
Online Access: | http://dx.doi.org/10.1007/978-1-4614-3308-8 Перейти в каталог НБ ТГУ |
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