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...
Enregistré dans:
| Auteur principal: | |
|---|---|
| Format: | Livre numérique |
| Langue: | Anglais |
| Publié: |
New York, NY :
Springer New York
[20..].
Cham : Springer Nature |
| Édition: | 1st ed. 2012. |
| Collection: | Springer Theses, Recognizing Outstanding Ph.D. Research
|
| Accès en ligne: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Note: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • On the Formation of the Most Massive Stars in the Galaxy, doctoral thesis accepted by Universidad Nacional Autónoma de México, Roberto J. Galván-Madrid, New York, Springer, 2012, 1 vol. (XIII-122 p.), Springer theses, 978-1-4614-3307-1 • On the Formation of the Most Massive Stars in the Galaxy, Texte imprimé, 9781461433095 • On the Formation of the Most Massive Stars in the Galaxy, doctoral thesis accepted by Universidad Nacional Autónoma de México, Roberto J. Galván-Madrid, New York, Springer, 2012, 1 vol. (XIII-122 p.), Springer theses, 978-1-4614-3307-1 |
Table des matières:
- 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