Transient X-ray pulsar V0332+53: pulse phase-resolved spectroscopy and the reflection model
Abstract
We present the results of the pulse phase- and luminosity-resolved spectroscopy of the transient X-ray pulsar V0332+53, performed for the first time in a wide luminosity range (1-40)x10^{37} erg/s during a giant outburst observed by the RXTE observatory in Dec 2004 - Feb 2005. We characterize the spectra quantitatively and built the detailed "three-dimensional" picture of spectral variations with pulse phase and throughout the outburst. We show that all spectral parameters are strongly variable with the pulse phase, and the pattern of this variability significantly changes with luminosity directly reflecting the associated changes in the structure of emission regions and their beam patterns. Obtained results are qualitatively discussed in terms of the recently developed reflection model for the formation of cyclotron lines in the spectra of X-ray pulsars.
Keywords
Cite
@article{arxiv.1502.03783,
title = {Transient X-ray pulsar V0332+53: pulse phase-resolved spectroscopy and the reflection model},
author = {A. A. Lutovinov and S. S. Tsygankov and V. F. Suleimanov and A. A. Mushtukov and V. Doroshenko and D. I. Nagirner and J. Poutanen},
journal= {arXiv preprint arXiv:1502.03783},
year = {2015}
}
Comments
12 pages, 10 figures, 3 tables, accepted for publication in MNRAS