{ "id": "2111.11953", "version": "v1", "published": "2021-11-23T15:46:58.000Z", "updated": "2021-11-23T15:46:58.000Z", "title": "Timing and Spectral Analysis of HMXB OAO 1657-415 with NuSTAR", "authors": [ "Prince Sharma", "Rahul Sharma", "Chetana Jain", "Anjan Dutta" ], "comment": "Accepted for publication in MNRAS", "doi": "10.1093/mnras/stab3436", "categories": [ "astro-ph.HE" ], "abstract": "This work presents a comprehensive timing and spectral analysis of high-mass X-ray binary pulsar, OAO 1657-415 by using the observation made with Nuclear Spectroscopic Telescope Array (NuSTAR) on June 2019. During this observation, OAO 1657-415 exhibited X-ray variability by a factor of about 3. X-ray pulsations at 37.03322(14) s were observed up to 70 keV. OAO 1657-415 was undergoing a spin-down phase with $\\dot{P} = 9(1) \\times 10^{-8}$ s s$^{-1}$. This is an order of about 100 larger than the long-term spin-up rate. The pulse profile evolved marginally during the observation. We have discussed the long-term pulse period history of the source spanning a time-base of 43 years, including the latest Fermi/GBM data. The 3-70 keV source spectrum is described by a partially covered cutoff power-law, an Fe K$_{\\alpha}$ line at 6.4 keV and a Compton shoulder at 6.3 keV. We report the presence of a cyclotron absorption feature around 40 keV, which is indicative of a surface magnetic field strength of $3.59 \\pm 0.06 \\ (1 + z)^{-1} \\times 10^{12}$ and $3.29_{-0.22}^{+0.23} \\ (1 + z)^{-1} \\times 10^{12}$ G. This work shows the first robust presence of cyclotron absorption feature in the source.", "revisions": [ { "version": "v1", "updated": "2021-11-23T15:46:58.000Z" } ], "analyses": { "keywords": [ "spectral analysis", "hmxb oao", "cyclotron absorption feature", "surface magnetic field strength", "high-mass x-ray binary pulsar" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }