Broad-band analysis of X-ray pulsar 2S 1845024
arXiv:2110.06642 · doi:10.1051/0004-6361/202141608
Abstract
We present results of detailed investigation of the poorly studied X-ray pulsar 2S 1845024 based on the data obtained with observatory during the type I outburst in 2017. Neither pulse phase-averaged, nor phase-resolved spectra of the source show evidence for a cyclotron absorption feature. We also used the data obtained from other X-ray observatories (, and ) to study the spectral properties as a function of orbital phase. The analysis revealed a high hydrogen column density for the source reaching 10 cm around the periastron. Using high-quality data we were able to obtain an accurate localization of 2S 1845024 at R.A. = 184816.8 and Dec. = 225'25".1 (J2000) that allowed us to use infrared (IR) data to roughly classify the optical counterpart of the source as an OB supergiant at the distance of 15 kpc.
arXiv comment8 pages, 8 figures, 6 tables, accepted for publication in A&A
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