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...
| Main Author: | Galván-Madrid, Roberto J. |
|---|---|
| Other Authors: | SpringerLink (Online Service) |
| Format: | eBook |
| Language: | English |
| Published: |
New York, NY :
Springer,
©2012.
|
| Physical Description: |
1 online resource : illustrations. |
| Series: |
Springer theses.
|
| Subjects: |
Stars
-- Formation.
|
CMU Electronic Access
Electronic Resource Click Here| Location | Call Number: | Status |
|---|---|---|
| CMU Electronic Access | Available |