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Просмотр по автору "Rauch T."

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Absorption features in the spectra of X-ray bursting neutron stars

Rauch T.; Suleimanov V.; Werner K. (2008)

Context. The discovery of photospheric absorption lines in XMM-Newton spectra of the X-ray bursting neutron star in EXO0748-676 by Cottam and collaborators allows us to constrain the neutron star mass-radius ratio from the ...
Absorption features in the spectra of x-ray bursting neutron stars

Suleimanov V.; Rauch T.; Werner K. (2012)

The photospheric absorption lines in the XMM-Newton spectra of the X-ray bursting neutron star EXO0748-676 were found by Cottam et al. (2002)1 and identified as the n = 2-3 transitions in hydrogen and helium like ions of ...
First high-resolution Chandra LETGS spectrum of the transient supersoft X-ray source RX J0513.9-6951

Burwitz V.; Reinsch K.; Greiner J.; Rauch T.; Suleimanov V.; Walter F.; Mennickent R.; Predehl P. (2007)

The transient luminous soft X-ray source RX J0513.9-6951 in the large magellanic cloud is a key object within the class of accreting binary supersoft X-ray sources. In this system, mass-transfer is thought to occur close ...
Non-LTE models for neutron star atmospheres and supernova-fallback disks

Werner K.; Nagel T.; Rauch T.; Suleimanov V. (2007)

We describe our recent progress in modeling supernova-fallback disks and neutron star (NS) atmospheres. We present a first detailed spectrum synthesis calculation of a SN-fallback disk composed of iron. We assume a thin ...
On the relevance of Compton scattering for the soft X-ray spectra of hot DA white dwarfs

Suleimanov V.; Madej J.; Drake J.; Rauch T.; Werner K. (2006)

Aims. We re-examine the effects of Compton scattering on the emergent spectra of hot DA white dwarfs in the soft X-ray range. Earlier studies have implied that sensitive X-ray observations at wavelengths λ < 50 Å might be ...
The double-degenerate nucleus of the planetary nebula TS01: A close binary evolution showcase

Tovmassian G.; Yungelson L.; Rauch T.; Suleimanov V.; Napiwotzki R.; Stasińska G.; Tomsick J.; Wilms J.; Morisset C.; Pẽa M.; Richer M. (2010)

We present a detailed investigation of SBS1150+599A, a close binary star hosted by the planetary nebula PNG135.9+55.9 (TS 01). The nebula, located in the Galactic halo, is the most oxygen-poor known to date and is the only ...

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Просмотр по автору "Rauch T."

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