{
  "id": "2010.15341",
  "version": "v1",
  "published": "2020-10-29T03:38:25.000Z",
  "updated": "2020-10-29T03:38:25.000Z",
  "title": "A supernova remnant associated with a nascent black hole low-mass X-ray binary",
  "authors": [
    "N. I. Maxted",
    "A. J. Ruiter",
    "K. Belczynski",
    "I. R. Seitenzahl",
    "R. M. Crocker"
  ],
  "comment": "4 pages text + 2 figures (8 pages total). To be submitted. Comments and feedback welcome!",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "Energy released when the core of a high-mass star collapses into a black hole often powers an explosion that creates a supernova remnant. Black holes have limited windows of observability, and consequently are rarely identified in association with supernova remnants. Analysing multi-messenger data, we show that MAXI J1535-571 is the black hole produced in the stellar explosion that gave rise to the supernova remnant G323.7-1.0, making it the first case of an association between a black hole low-mass X-ray binary and a supernova remnant. Given this connection, we can infer from our modelling that the progenitor system was a close binary whose primary star had an initial mass of approx. 23-35 solar masses with a companion star about 10 times less massive.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-10-29T03:38:25.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "black hole low-mass x-ray binary",
      "nascent black hole low-mass x-ray",
      "supernova remnant",
      "high-mass star collapses"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}