{
  "annotation_id": "43c2cdc8-3219-4df3-b3b7-ea9d0684d72a",
  "date_created": "2026-03-02T18:00:53.452000Z",
  "date_modified": "2026-03-02T18:00:53.452000Z",
  "file_hash": "2ec693bf36d4199197ae2c15d147edc75a5df538150b28e1a49732486431d654",
  "private": false,
  "record": {
    "abstract": "We present the timing and spectral properties of the transient Be/X-ray\nbinary pulsar 3A 0535+262 during quiescence using three observations with the\nnarrow field imaging instruments (NFI) of BeppoSAX. Assuming a distance of 2\nkpc for this system, the 2-10 keV X-ray luminosities measured from the three\nobservations are in the range of 1.5-4.0 $\\times$ 10$^{33}$ erg s$^{-1}$,\nindicating a very low rate of accretion. We report the detection of pulsations\nat a very low luminosity of 2 $\\times$ 10$^{33}$ erg s$^{-1}$ during one of the\nthree observations, though at this accretion rate the system is expected to be\nin the centrifugally inhibited regime. The X-ray spectra for the unpulsed\nobservations are best modeled as power law type while a combined model of power\nlaw and black-body is required to fit the pulsed spectrum.",
    "arxiv_id": "physics/0410255",
    "authors": [
      "U. Mukherjee",
      "B. Paul"
    ],
    "categories": [
      "physics.data-an",
      "astro-ph"
    ],
    "doi": "10.1051/0004-6361:20041665",
    "title": "X-ray properties of the transient pulsar 3A 0535+262 in quiescence",
    "url": "https://arxiv.org/abs/physics/0410255"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "d54f23de-5a86-49f0-ac21-86051a9c9186",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}