X- And γ-Ray Pulsations Of The Nearby Radio-Faint PSR J1741–2054
- Istituto Nazionale di Astrofisica (INAF), Milano (Italy)
- Istituto Nazionale di Astrofisica (INAF), Milano (Italy); Univ. of California, Santa Cruz, CA (United States). Santa Cruz Inst. for Particle Physics
- Univ. of California, Santa Cruz, CA (United States). Santa Cruz Inst. for Particle Physics; City Univ. of Hong Kong (China)
- Istituto Nazionale di Astrofisica (INAF), Milano (Italy); Istituto Nazionale di Fisica Nucleare (INFN), Pavia (Italy)
- Univ. of Virginia, Charlottesville, VA (United States)
- Istituto Nazionale di Astrofisica (INAF), Milano (Italy); Istituto Nazionale di Fisica Nucleare (INFN), Pavia (Italy); Univ. degli Studi di Pavia (Italy)
- Univ. of Virginia, Charlottesville, VA (United States); Univ. of Alberta, Edmonton, AB (Canada)
- Columbia Univ., New York, NY (United States). Columbia Astrophysics Lab.; Arecibo Observatory, PR (United States)
The results of a deep XMM-Newton observation of the radio-faint γ-ray pulsar J1741–2054 and its nebula together with the analysis of five years of Fermi Large Area Telescope (LAT) data are reported. The X-ray spectrum of the pulsar is consistent with an absorbed power law plus a blackbody, originating at least partly from the neutron star cooling. The nebular emission is consistent with that of a synchrotron pulsar wind nebula, with hints of spatial spectral variation. We extended the available Fermi LAT ephemeris and folded the γ-ray and X-ray data. We detected X-ray pulsations from the neutron star: both the thermal and non-thermal components are ~35%-40% pulsed, with phase-aligned maxima. A sinusoid fits the thermal-folded profile well. A 10 bin phase-resolved analysis of the X-ray emission shows softening of the non-thermal spectrum during the on-pulse phases. The radio, X-ray, and γ-ray light curves are single-peaked, not phase-aligned, with the X-ray peak trailing the γ-ray peak by more than half a rotation. Spectral considerations suggest that the most probable pulsar distance is in the 0.3-1.0 kpc range, in agreement with the radio dispersion measure.
- Research Organization:
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Sponsoring Organization:
- USDOE
- Grant/Contract Number:
- AC02-76SF00515
- OSTI ID:
- 1356463
- Journal Information:
- The Astrophysical Journal, Vol. 790, Issue 1; ISSN 0004-637X
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
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