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...
Shranjeno v:
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| Format: | Livre numérique |
| Jezik: | Anglais |
| Izdano: |
New York, NY :
Springer New York
[20..].
Cham : Springer Nature |
| Izdaja: | 1st ed. 2012. |
| Serija: | Springer Theses, Recognizing Outstanding Ph.D. Research
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| Online dostop: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Sporočilo: |
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 |
| Izvleček: | 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 Large Array (VLA) studies of massive star formation regions in the early stages of ionization, as well as an analysis of numerical simulations of the evolution of these young HII regions. The results favor a picture in which very massive stars form in accretion flows that are partially ionized and that keep accreting material from their environment.The American Astronomical Society selected Roberto Galvan-Madrid as a prize winner for The Rodger Doxsey Travel Prize in 2010 |
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| Opis knjige/članka: | Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| ISBN: | 9781461433088 |
| ISSN: | 2190-5061 |
| Dostop: | Accès en ligne pour les établissements français bénéficiaires des licences nationales Accès soumis à abonnement pour tout autre établissement Conditions particulières de réutilisation pour les bénéficiaires des licences nationales. https://www.licencesnationales.fr/springer-nature-ebooks-contrat-licence-ln-2017 |