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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 |
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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 |
MARC
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| 001 | 978-1-4614-3308-8 | ||
| 003 | DE-He213 | ||
| 005 | 20220117024521.0 | ||
| 007 | cr nn 008mamaa | ||
| 008 | 120608s2012 xxu| s |||| 0|eng d | ||
| 020 | |a 9781461433088 |9 978-1-4614-3308-8 | ||
| 024 | 7 | |a 10.1007/978-1-4614-3308-8 |2 doi | |
| 050 | 4 | |a QB1-991 | |
| 072 | 7 | |a PG |2 bicssc | |
| 072 | 7 | |a SCI004000 |2 bisacsh | |
| 072 | 7 | |a PG |2 thema | |
| 082 | 0 | 4 | |a 520 |2 23 |
| 082 | 0 | 4 | |a 500.5 |2 23 |
| 100 | 1 | |a Galván-Madrid, Roberto J. |e author. |4 aut |4 http://id.loc.gov/vocabulary/relators/aut | |
| 245 | 1 | 0 | |a On the Formation of the Most Massive Stars in the Galaxy |h [electronic resource] / |c by Roberto J. Galván-Madrid. |
| 250 | |a 1st ed. 2012. | ||
| 264 | 1 | |a New York, NY : |b Springer New York : |b Imprint: Springer, |c 2012. | |
| 300 | |a XIII, 122 p. 49 illus., 23 illus. in color. |b online resource. | ||
| 336 | |a text |b txt |2 rdacontent | ||
| 337 | |a computer |b c |2 rdamedia | ||
| 338 | |a online resource |b cr |2 rdacarrier | ||
| 347 | |a text file |b PDF |2 rda | ||
| 490 | 1 | |a Springer Theses, Recognizing Outstanding Ph.D. Research, |x 2190-5061 | |
| 505 | 0 | |a 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. | |
| 520 | |a 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. | ||
| 650 | 0 | |a Astronomy. | |
| 650 | 1 | 4 | |a Astronomy, Cosmology and Space Sciences. |
| 710 | 2 | |a SpringerLink (Online service) | |
| 773 | 0 | |t Springer Nature eBook | |
| 776 | 0 | 8 | |i Printed edition: |z 9781461433095 |
| 776 | 0 | 8 | |i Printed edition: |z 9781461433071 |
| 830 | 0 | |a Springer Theses, Recognizing Outstanding Ph.D. Research, |x 2190-5061 | |
| 856 | 4 | 0 | |u https://doi.uam.elogim.com/10.1007/978-1-4614-3308-8 |z Texto Completo |
| 912 | |a ZDB-2-PHA | ||
| 912 | |a ZDB-2-SXP | ||
| 950 | |a Physics and Astronomy (SpringerNature-11651) | ||
| 950 | |a Physics and Astronomy (R0) (SpringerNature-43715) | ||