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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...
| Clasificación: | Libro Electrónico |
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| Autor principal: | |
| Autor Corporativo: | |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
New York, NY :
Springer New York : Imprint: Springer,
2012.
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| Edición: | 1st ed. 2012. |
| Colección: | Springer Theses, Recognizing Outstanding Ph.D. Research,
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| Temas: | |
| Acceso en línea: | Texto Completo |
Tabla de Contenidos:
- Foreword by Prof. Luis F. Rodriguez (CRyA-UNAM) and Dr. Qizhou Zhang (Harvard-Smithsonian Center for Astrophysics).-Chapter 1: Introduction to the Scientific Problem
- Chapter 2: A MSFR at the Onset of Ionization: W33A
- Chapter 3: A MSFR with young UC and HC HII Regions: G20.08N
- Chapter 4: Time Variability of HII Regions: A Signature of Accretion?
- Chapter 5: Time Variability of HII Regions in Numerical Simulations of MSFR
- Chapter 6: Conclusions
- Bibliography
- Appendix I: Radio and (Sub)millimeter Interferometers
- Appendix II: Molecular-line Emission
- Appendix III: Ionized-Gas Emission
- Index.