SIMBAD references

2010A&A...518A..46T - Astronomy and Astrophysics, volume 518, A46-46 (2010/7-2)

The energy spectrum of anomalous X-ray pulsars and soft gamma-ray repeaters.

TRUEMPER J.E., ZEZAS A., ERTAN U. and KYLAFIS N.D.

Abstract (from CDS):

Anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs) exhibit characteristic X-ray luminosities (both soft and hard) of around 1035 erg/s and characteristic power-law, hard X-ray spectra extending to about 200 keV. Two AXPs also exhibit pulsed radio emission. Assuming that AXPs and SGRs accrete matter from a fallback disk, we attempt to explain both the soft and the hard X-ray emission as the result of the accretion process. We also attempt to explain their radio emission or the lack of it. We test the hypothesis that the power-law, hard X-ray spectra are produced in the accretion flow mainly by bulk-motion Comptonization of soft photons emitted at the neutron star surface. Fallback disk models invoke surface dipole magnetic fields of 1012 - 1013G, which is what we assume here. Unlike normal X-ray pulsars, for which the accretion rate is highly super-Eddington, the accretion rate is approximately Eddington in AXPs and SGRs and thus the bulk-motion Comptonization operates efficiently. As an illustrative example we reproduce both the hard and the soft X-ray spectra of AXP 4U 0142+61 well using the XSPEC package compTB. Our model seems to explain both the hard and the soft X-ray spectra of AXPs and SGRs, as well as their radio emission or the lack of it, in a natural way. It might also explain the short bursts observed in these sources. On the other hand, it cannot explain the giant X-ray outbursts observed in SGRs, which may result from the conversion of magnetic energy in local multipole fields.

Abstract Copyright:

Journal keyword(s): pulsars: individual: 1E 1841-045 - pulsars: individual: 1RXS J1708-4009 - pulsars: individual: 4U 0142+61 - X-rays: stars - stars: magnetic fields

Simbad objects: 8

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2021.03.09-09:59:02

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