AX J1910.7+0917: the slowest X-ray pulsar

Journal
Date Issued
2017
Author(s)
•
•
Esposito, P.
•
•
Postnov, K.
DOI
Abstract
Pulsations from the high-mass X-ray binary AX J1910.7+0917 were discovered during Chandra observations performed in 2011. We report here more details on this discovery and discuss the source nature. The period of the X-ray signal is P = 36200 ± 110 s, with a pulsed fraction, PF, of 63 ± 4 per cent. Given the association with a massive B-type companion star, we ascribe this long periodicity to the rotation of the neutron star (NS), making AX J1910.7+0917 the slowest known X-ray pulsar. We also report on the spectroscopy of XMM-Newton observations that serendipitously covered the source field, resulting in a highly absorbed (column density almost reaching 1023 cm-2), power-law X-ray spectrum. The X-ray flux is variable on a time-scale of years, spanning a dynamic range ≳ 60. The very long NS spin period can be explained within a quasi-spherical settling accretion model that applies to low luminosity, wind-fed, X-ray pulsars.
Volume
469
Issue
3
Start page
3056
Uri
Url
Issn Identifier
0035-8711
Ads BibCode
2017MNRAS.469.3056S
Rights
open.access
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