{ "id": "2404.02782", "version": "v1", "published": "2024-04-03T14:53:28.000Z", "updated": "2024-04-03T14:53:28.000Z", "title": "AstroSat View of the Neutron Star Low-mass X-Ray Binary GX 5-1", "authors": [ "Shyam Prakash V P", "Vivek K. Agrawal" ], "comment": "11 pages, 5 figures, 4 tables", "categories": [ "astro-ph.HE" ], "abstract": "We present the spectral and timing study of the bright NS-LMXB GX 5-1 using \\textit{\\textit{AstroSat}/LAXPC} and \\textit{SXT} observations conducted in the year 2018. During the observation, the source traces out the complete HB and NB of the Z-track in the HID. Understanding the spectral and temporal evolution of the source along the 'Z' track can probe the accretion process in the vicinity of a neutron star. Spectral analysis was performed in the 0.7-20 keV energy range for different segments in the HID using a multi-temperature disc black body with an average temperature, $kT_{in} \\sim$0.46 and a thermal Comptonization model. It is found that the optical depth of the corona drops from $\\sim$6.68 in HB to $\\sim$2.74 in NB. The Timing analysis using the LAXPC instrument indicates the presence of quasi-periodic oscillations in HB, NB, and the hard apex of the Z-track. The observed QPO frequencies are similar to the characteristic frequencies of horizontal branch and normal branch oscillations. The HBO frequency increase from $\\sim$12-46 Hz towards the hard apex. The timing studies conducted in soft and hard band indicate the association of HBO and NBO origin with the non-thermal component. Further research could explore the implications of this relationship for understanding the dynamics of accretion onto neutron stars.", "revisions": [ { "version": "v1", "updated": "2024-04-03T14:53:28.000Z" } ], "analyses": { "keywords": [ "neutron star low-mass x-ray binary", "star low-mass x-ray binary gx", "astrosat view", "hard apex", "multi-temperature disc black body" ], "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable" } } }