In this study, X-ray spectral and pulse timing analysis of the high mass X-ray binary (HMXB) pulsar 4U 1907+09, based on the observations with RXTE are presented. Spin rate measurements indicate a new spin-down episode with a rate close to the previous steady spin-down rate. Orbital phase resolved spectroscopy reveals that the Hydrogen column density varies through the orbit reaching to its maximum value just after periastron. A slight spectral softening with increasing luminosity is also observed.
@article{arxiv.1104.4898,
title = {Recent Spin Rate Measurements of 4U 1907+09},
author = {S. Sahiner and S. C. Inam and A. Baykal},
journal= {arXiv preprint arXiv:1104.4898},
year = {2015}
}
Comments
3 pages, 1 figure, Conference proceeding of "Astrophysics of Neutron Stars 2010 -- a conference in honor of M. Ali Alpar", 2-6 August 2010, Cesme, Izmir, Turkey