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Obscuring Supersoft X-ray Sources in Stellar Winds
| Content Provider | Semantic Scholar |
|---|---|
| Author | Nielsen, Mikkel Dominik, Carsten Nelemans, G. A. |
| Copyright Year | 2011 |
| Abstract | We investigate the possibility of obscuring supersoft X-ray sources in the winds of companion stars. We derive limits on the amount of circumstellar material needed to fully obscure a ‘canonical’ supersoft X-ray source in the Large Magellanic Cloud, as observed with the Chandra X-ray Observatory. |
| Starting Page | 140 |
| Ending Page | 144 |
| Page Count | 5 |
| File Format | PDF HTM / HTML |
| DOI | 10.1017/S1743921312014883 |
| Volume Number | 281 |
| Alternate Webpage(s) | https://pure.uva.nl/ws/files/2061154/142894_Obscuring_Supersoft_X_ray_Sources_in_Stellar_Winds.pdf |
| Alternate Webpage(s) | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/C229FE220186DAA4736340A133D19BE6/S1743921312014883a.pdf/obscuring_supersoft_xray_sources_in_stellar_winds.pdf |
| Alternate Webpage(s) | https://arxiv.org/pdf/1109.5866v1.pdf |
| Alternate Webpage(s) | https://doi.org/10.1017/S1743921312014883 |
| Language | English |
| Access Restriction | Open |
| Content Type | Text |
| Resource Type | Article |