{
  "abstract": "We present a spectral analysis of the NuSTAR and NICER observations of the accreting millisecond X-ray pulsar IGR J17062-6143, performed in 2022. The source remained in the hard spectral state during these observations, with a luminosity of about $\\sim$0.13-0.14 percent of the Eddington luminosity. The continuum emission of the NuSTAR spectrum is entirely dominated by a power-law component or by Comptonized emission of disc photons by a plasma with a high electron temperature ($\\gtrsim100$ keV). The NuSTAR spectrum also reveals clear evidence of disc reflection, a broad Fe K line around 6-8 keV, and a Compton hump peaking at 20 keV, irrespective of the choice of the continuum models. Our spectral studies suggest a disk extending close to the neutron star surface ($\\sim$6-20 $R_{\\rm g}$) at low inclination angle ($\\sim41$ degrees), as revealed by the self-consistent relativistic reflection model, relxill. In addition, we detected type-II-like bursts for the first time in the NICER observation of this source. Light curve profiles of type-II-like bursts exhibit different patterns, mostly associated with the so-called mode-0 and transition from mode-0 to mode-1 type-II bursts. The energy spectra of the persistent (pre-burst) and burst emission are well described by an absorbed Comptonization component, scattering disk- and blackbody-distributed photons, respectively, by a corona with a temperature of 1-3 keV. Although the origin of the type-II-like burst is not very clear, it has been possibly linked to disk-magnetosphere interaction of the accretion flow.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2606.23156",
  "author_total": 5,
  "authors": [
    {
      "name": "Aditya Sow Mondal"
    },
    {
      "name": "Mahasweta Bhattacharya"
    },
    {
      "name": "Swarnendu Jana"
    },
    {
      "name": "Biplab Raychaudhuri"
    },
    {
      "name": "Gulab C. Dewangan"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/0r9hcs7bnqy10.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2606.23156",
  "fulltext_url": null,
  "id": "0r9hcs7bnqy10",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2606.23156",
  "language": null,
  "licence": "CC-BY-NC-ND-4.0",
  "licence_label": "CC BY-NC-ND 4.0",
  "licence_source": "article",
  "licence_url": "http://creativecommons.org/licenses/by-nc-nd/4.0/",
  "metadata_licence": "CC0-1.0",
  "native_subjects": [
    [
      "arxiv",
      "astro-ph.HE"
    ],
    [
      "openalex",
      "3103|Astrophysical Phenomena and Observations"
    ]
  ],
  "openalex": "W7165640681",
  "pdf_url": "https://arxiv.org/pdf/2606.23156",
  "pmcid": null,
  "pmid": null,
  "published": "2026-10-26",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/0r9hcs7bnqy10.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T12:35:35Z",
      "native_id": "2606.23156",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2606.23156"
    }
  ],
  "subjects": [
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.HE",
      "subfield": "high-energy-astrophysics"
    }
  ],
  "title": "On the assessment of the disk truncation and detection of type-II-like bursts from the accreting millisecond X-ray Pulsar IGR J17062-6143",
  "title_text": "On the assessment of the disk truncation and detection of type-II-like bursts from the accreting millisecond X-ray Pulsar IGR J17062-6143",
  "type": "preprint",
  "updated_at": "2026-10-30T12:35:35Z",
  "url": "https://research.draconitic.com/paper/0r9hcs7bnqy10",
  "venue": "arXiv",
  "versions": []
}