Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra
We report the detection from four symbiotic stars that were not known to be X-ray sources. These four object show a β-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 wi...
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| Autores principales: | Nuñez, N.E., Luna, G.J.M., Pillitteri, I., Mukai, K. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046361_v565_n_p_Nunez |
| Aporte de: |
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