Non-LTE model atmospheres for supersoft X-ray sources

Details Non-LTE model atmospheres for supersoft X-ray sources Non-LTE model atmospheres for supersoft X-ray sources

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010an....331..146r&link_type=abstract

Astronomische Nachrichten, Vol.331, Issue 2, p.146

Astronomy and Astrophysics

Astronomy

5

Novae, Cataclysmic Variables, Stars: Agb And Post-Agb, Stars: Individual (Lsv 4621, H 1504+65, V4743 Sgr, Exo 0748-676), White Dwarfs, X-Rays: Stars

Scientific paper

In the last decade, X-ray observations of hot stellar objects became available with unprecedented resolution and S/N ratio. For an adequate interpretation, fully metal-line blanketed Non-LTE model-atmospheres are necessary. The Tübingen Non-LTE Model Atmosphere Package (TMAP) can calculate such model atmospheres at a high level of sophistication. Although TMAP is not especially designed for the calculation of spectral energy distributions (SEDs) at extreme photospheric parameters, it can be employed for the spectral analysis of burst spectra of novae like V4743 Sgr or line identifications in observations of neutron stars with low magnetic fields in low-mass X-ray binaries (LMXBs) like EXO 0748-676.

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