| タイトル | Symbiotic Stars in X-rays. II. Faint Sources Detected with XMM-Newton and Chandra |
| 本文（外部サイト） | http://hdl.handle.net/2060/20150011656 |
| 著者（英） | Nunez, N. E.; Mukai, K.; Luna, G. J. M.; Pillitteri, I. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2014-05-16 |
| 言語 | eng |
| 内容記述 | We report the detection from four symbiotic stars that were not known to be X-ray sources. These four object show a -type X-ray spectrum, that is, their spectra can be modeled with an absorbed optically thin thermal emission with temperatures of a few million degrees. Photometric series obtained with the Optical Monitor on board XMM-Newton from V2416 Sgr and NSV 25735 support the proposed scenario where the X-ray emission is produced in a shock-heated region inside the symbiotic nebulae. |
| NASA分類 | Astronomy; Astrophysics |
| レポートNO | GSFC-E-DAA-TN23917 |
| 権利 | Copyright, Distribution under U.S. Government purpose rights |
