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19 April 2024 |
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Supersoft X-ray Sources. Parameters of Stellar Atmospheres | | A. Ibragimov
; V. Suleimanov
; A. Vikhlinin
; N. Sakhibullin
; | | Date: |
16 Mar 2006 | | Journal: | Astron.Rep. 47 (2003) 186 | | Abstract: | ROSAT spectra of 11 supersoft X-ray sources (RX J0439.8-6809, RX J0513.9-6951, RX J0527.8-6954, CAL 87, CAL 83, 1E 0035.4-7230, RX J0048.4-7332, 1E 0056.8-7154, RX J0019.8 +2156, RX J0925.7-4758, AG Draconis) are approximated with theoretical spectra obtained in LTE models for the atmospheres of hot white dwarfs with line blanketing. The confidence intervals of parameters derived from these approximations $ T_{
m eff}$, $log g$, $N_H$, and $R^2/d^2$ are determined. The results are compared with predictions for a model with stable/recurrent thermonuclear burning on the white-dwarf surface. | | Source: | arXiv, astro-ph/0603429 | | Services: | Forum | Review | PDF | Favorites | |
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