{ "id": "1602.08287", "version": "v1", "published": "2016-02-26T11:58:11.000Z", "updated": "2016-02-26T11:58:11.000Z", "title": "Effects of variability of X-ray binaries on the X-ray luminosity functions of Milky Way", "authors": [ "Nazma Islam", "Biswajit Paul" ], "comment": "Accepted for publication in New Astronomy", "categories": [ "astro-ph.HE" ], "abstract": "The X-ray luminosity functions of galaxies have become a useful tool for population studies of X-ray binaries in them. The availability of long term light-curves of X-ray binaries with the All Sky X-ray Monitors opens up the possibility of constructing X-ray luminosity functions, by also including the intensity variation effects of the galactic X-ray binaries. We have constructed multiple realizations of the X-ray luminosity functions (XLFs) of Milky Way, using the long term light-curves of sources obtained in the 2-10 keV energy band with the RXTE-ASM. The observed spread seen in the value of slope of both HMXB and LMXB XLFs are due to inclusion of variable luminosities of X-ray binaries in construction of these XLFs as well as finite sample effects. XLFs constructed for galactic HMXBs in the luminosity range 10^{36} - 10^{39} erg/sec is described by a power-law model with a mean power-law index of -0.48 and a spread due to variability of HMXBs as 0.19. XLFs constructed for galactic LMXBs in the luminosity range 10^{36} - 10^{39} erg/sec has a shape of cut-off power-law with mean power-law index of -0.31 and a spread due to variability of LMXBs as 0.07.", "revisions": [ { "version": "v1", "updated": "2016-02-26T11:58:11.000Z" } ], "analyses": { "keywords": [ "x-ray binaries", "milky way", "mean power-law index", "long term light-curves", "variability" ], "publication": { "doi": "10.1016/j.newast.2016.02.008" }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1424512 } } }