Non-LTE Models for Neutron Star Atmospheres and Supernova-Fallback Disks
Abstract
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 disk with a radial structure described by the alpha-disk model. The vertical structure and emission spectrum are computed self-consistently by solving the structure equations simultaneously with the radiation transfer equations under non-LTE conditions. We describe the properties of a specific disk model and discuss various effects on the emergent UV/optical spectrum. We investigate Compton scattering effects on the thermal spectrum of NSs. In addition, we constructed a new generation of metal line-blanketed non-LTE model atmospheres for NSs. It is compared to X-ray burst spectra of EXO0748-676. It is possible that the gravitational redshift, deduced from absorption lines, is lower (z=0.24) than hitherto assumed (z=0.35). Accordingly, this would result in NS mass and radius lower limits of M>1.63Msun and R>13.8 km.
Keywords
Cite
@article{arxiv.astro-ph/0612425,
title = {Non-LTE Models for Neutron Star Atmospheres and Supernova-Fallback Disks},
author = {K. Werner and T. Nagel and T. Rauch and V. Suleimanov},
journal= {arXiv preprint arXiv:astro-ph/0612425},
year = {2008}
}
Comments
Accepted for publication in Advances in Space Research