| 书目名称 | Stellar Disk Evolution and Gaseous Disk Turbulence of Dwarf Irregular Galaxies |
| 编辑 | Hong-Xin Zhang |
| 视频video | |
| 概述 | Nominated as an outstanding thesis by University of Chinese Academy of Sciences.Establishes the "outside-in" disk growth mode for most nearby dwarf irregular galaxies.Disproves the existence of a corr |
| 丛书名称 | Springer Theses |
| 图书封面 |  |
| 描述 | This book focuses on the stellar disk evolution and gas disk turbulence of the most numerous galaxies in the local Universe – the dwarf galaxies. The “outside-in” disk shrinking mode was established for a relatively large sample of dwarf galaxies for the first time, and this is in contrast to the “inside-out” disk growth mode found for spiral galaxies. Double exponential brightness profiles also correspond to double exponential stellar mass profiles for dwarf galaxies, which is again different from most spiral galaxies. The cool gas distribution in dwarf galaxies was probed with the spatial power spectra of hydrogen iodide (HI) gas emission, and provided indirect evidence that inner disks of dwarf galaxies have proportionally more cool gas than outer disks. The finding that no correlation exists between gas power spectral indices and star formation gave important constraints on the relation between turbulence and star formation in dwarf galaxies. |
| 出版日期 | Book 2016 |
| 关键词 | ‘‘inside-out‘‘ Disk Growth Scenario; Azimuthally-averaged Surface Photometry; Dwarf Irregular Galaxies |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-3-662-52867-9 |
| isbn_softcover | 978-3-662-57089-0 |
| isbn_ebook | 978-3-662-52867-9Series ISSN 2190-5053 Series E-ISSN 2190-5061 |
| issn_series | 2190-5053 |
| copyright | Springer-Verlag Berlin Heidelberg 2016 |
发表于 2025-3-21 18:45:50
