{ "id": "1704.01335", "version": "v1", "published": "2017-04-05T09:45:17.000Z", "updated": "2017-04-05T09:45:17.000Z", "title": "The Black Hole Candidate LSI+61303", "authors": [ "M. Massi", "S. Migliari", "M. Chernyakova" ], "comment": "5 pages, 4 figures, MNRAS accepted", "doi": "10.1093/mnras/stx778", "categories": [ "astro-ph.HE" ], "abstract": "In recent years, fundamental relationships for the black hole X-ray binaries have been established between their X-ray luminosity $L_X$ and the photon index $\\Gamma$ of their X-ray spectrum. For the moderate-luminosity regime, an anti-correlation between $\\Gamma$ and $L_X$ has been observed. In this article, aimed to verify if the moderate luminous X-ray binary system LSI +61303 is a black hole, we analyse $Swift$ observations of LSI +61303. We compare the derived $L_X$ vs $\\Gamma$ distribution, first with the statistical trend for black hole X-ray binaries, then with the trend of the pulsar PSR B1259-63, and finally with the individual trends of the black hole X-ray binaries Swift J1357.2-0933 and V404 Cygni. We find that the system PSR B1259-63 shows a positive correlation between $\\Gamma$ and $L_X$, whereas in contrast LSI +61303 shows the same anti-correlation as for black hole X-ray binaries. Moreover, the trend of LSI +61303 in the $L_X$/$L_{Eddington} - \\Gamma$ plane overlaps with that of the two black holes Swift J1357.2-0933 and V404 Cygni. All three systems, Swift J1357.2-0933, V404 Cygni and LSI +61303 well trace the last part of the evolution of accreting black holes at moderate-luminosity until their drop to quiescence.", "revisions": [ { "version": "v1", "updated": "2017-04-05T09:45:17.000Z" } ], "analyses": { "keywords": [ "black hole x-ray binaries", "black hole candidate", "x-ray binaries swift j1357", "x-ray binary system lsi", "hole x-ray binaries swift" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable" } } }