Models for the remnants of recurrent novae - III. Comparison with the X-ray observations of RS Ophiuchi (1985)
| العنوان: | Models for the remnants of recurrent novae - III. Comparison with the X-ray observations of RS Ophiuchi (1985) |
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| المؤلفون: | F. D. Kahn, M. F. Bode, Tim O'Brien |
| المصدر: | Monthly Notices of the Royal Astronomical Society. 255:683-693 |
| بيانات النشر: | Oxford University Press (OUP), 1992. |
| سنة النشر: | 1992 |
| مصطلحات موضوعية: | Physics, X-ray astronomy, Red giant, Astrophysics::High Energy Astrophysical Phenomena, X-ray, Astronomy, Astronomy and Astrophysics, Astrophysics, Light curve, Computational astrophysics, Space and Planetary Science, RS Ophiuchi, Astrophysics::Solar and Stellar Astrophysics, Circumstellar dust, Ejecta, Astrophysics::Galaxy Astrophysics |
| الوصف: | Ealiers papers of this series developed a model for the interaction of ejecta with a circumstellar medium which was principally applied to the 1985 outburst of the recurrent nova RS Ophiuchi. Here the X-ray emission predicted by this model is compared in detail to EXOSAT observations of the outburst. Fits to the first observations 55 days after outburst lead to values for model parameters which are consistent with existing estimates : outburst energy ⇒ 1.1 × 10 43 erg; ejecta mass ⇒ 1.1 × 10 -6 M ⊙ ; and mass-loss rate into the wind of the red giant component ⇒ 6 × 10 12 g/cm. Once these parameters are fixed the model predicts the subsequent evolution of the X-ray emission |
| تدمد: | 1365-2966 0035-8711 |
| URL الوصول: | https://explore.openaire.eu/search/publication?articleId=doi_________::5416793086f7389bd168b47ec7cafb23 https://doi.org/10.1093/mnras/255.4.683 |
| حقوق: | OPEN |
| رقم الأكسشن: | edsair.doi...........5416793086f7389bd168b47ec7cafb23 |
| قاعدة البيانات: | OpenAIRE |
| تدمد: | 13652966 00358711 |
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