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.
New York, NY : [2012] |
| Physical Description: |
1 online resource : illustrations. |
| Series: |
Springer theses.
|
| Subjects: |
Stars
-- Formation.
|
Table of Contents:
- Introduction to the Scientific Problem
- A MSFR at the Onset of Ionization: W33A
- A MSFR with Young UC and HC HII Regions: G20.08N
- Time Variability of HII Regions: A Signature of Accretion?
- Time Variability of HII Regions in Numerical Simulations of MSFR
- Conclusions.