| 书目名称 | On the Formation of the Most Massive Stars in the Galaxy |
| 编辑 | Roberto J. Galván-Madrid |
| 视频video | |
| 概述 | Presents results of Submillimeter Array (SMA) and Very Large Array (VLA) studies of massive-star formation regions in the early stages of ionization.Author has received the 2010 Doxey Prize, given out |
| 丛书名称 | Springer Theses |
| 图书封面 |  |
| 描述 | 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. |
| 出版日期 | Book 2012 |
| 关键词 | Accretion flow; Accretion signifiers; Gravitational collapse; HII regions; Ionization stages; Jets and ou |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-1-4614-3308-8 |
| isbn_softcover | 978-1-4614-3307-1 |
| isbn_ebook | 978-1-4614-3308-8Series ISSN 2190-5053 Series E-ISSN 2190-5061 |
| issn_series | 2190-5053 |
| copyright | Springer Science+Business Media New York 2012 |
发表于 2025-3-21 18:28:09
