Model atmospheres of X-ray bursting neutron stars
Abstract
We present an extended set of model atmospheres and emergent spectra of X-ray bursting neutron stars in low mass X-ray binaries. Compton scattering is taken into account. The models were computed in LTE approximation for six different chemical compositions: pure hydrogen and pure helium atmospheres, and atmospheres with a solar mix of hydrogen and helium and various heavy elements abundances; Z = 1, 0.3, 0.1, and 0.01 Zsolar, for three values of gravity, log g = 14.0, 14.3, and 14.6 and for 20 values of relative luminosity l = L/LEdd in the range 0.001-0.98. The emergent spectra of all models are fitted by diluted blackbody spectra in the observed RXTE/PCA band 3-20 keV and the corresponding values of color correction factors fc are presented. We also show how to use these dependencies to estimate the neutron star's basic parameters.
- Publication:
-
AstroPhysics of Neutron Stars 2010: A Conference in Honor of M. Ali Alpar
- Pub Date:
- September 2011
- DOI:
- 10.1063/1.3629513
- arXiv:
- arXiv:1010.0151
- Bibcode:
- 2011AIPC.1379..197S
- Keywords:
-
- spectral analysis;
- X-ray sources (astronomical);
- radiative transfer;
- redshift;
- 97.10.Ri;
- 98.70.Qy;
- 95.30.Jx;
- 98.62.Py;
- Luminosities;
- magnitudes;
- effective temperatures colors and spectral classification;
- X-ray sources;
- X-ray bursts;
- Radiative transfer;
- scattering;
- Distances redshifts radial velocities;
- spatial distribution of galaxies;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- 2 pages, 1 figure, conference "Astrophysics of Neutron Stars - 2010" in honor of M. Ali Alpar, Izmir, Turkey