2011MNRAS.412.1721V


Query : 2011MNRAS.412.1721V

2011MNRAS.412.1721V - Mon. Not. R. Astron. Soc., 412, 1721-1729 (2011/April-2)

The effect of the infrared excess from the Be star on inverse Compton gamma-ray production in PSR B1259-63/SS 2883.

VAN SOELEN B. and MEINTJES P.J.

Abstract (from CDS):

The binary system PSR B1259-63 consists of a 48-ms pulsar in a 3.4-yr orbit around a Be star, and unpulsed TeV gamma-ray emission has been detected near previous periastron passages. A likely source of the gamma-rays is the inverse Compton upscattering of target photons from the Be star by the ultrarelativistic electron/positron pulsar wind in the region of the plerion shock front. In this study, the effect of the infrared emission from the Be star's circumstellar disc on inverse Compton gamma-ray production in PSR B1259-63 is investigated by considering an isotropic photon/electron approximation. The modified photon density distribution is determined by using a curve of growth method fitted to previous optical and infrared observations. The inverse Compton scattering rate is calculated using the modified photon distribution and the exact scattering equation. It is shown that including the infrared emission increases the GeV gamma-ray flux by a factor of ≳ 2.

Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS

Journal keyword(s): radiation mechanisms: non-thermal - pulsars: individual: PSR B1259-63 - X-rays: binaries

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 LS I +61 303 HXB 02 40 31.6644419688 +61 13 45.593918580 11.27 11.61 10.75 10.19 9.55 B0Ve 903 2
2 V* X Per HXB 03 55 23.0777456088 +31 02 45.039836148 6.090 6.840 6.720     O9.5III 1037 0
3 * del Cen Be* 12 08 21.4976373 -50 43 20.738614 1.51 2.39 2.52 2.48 2.62 B2Vne 320 0
4 NAME Coalsack Nebula DNe 12 31 19 -63 44.6           ~ 275 0
5 CPD-63 2495 HXB 13 02 47.6544015048 -63 50 08.626970292 10.34 10.72 9.98 10.03   O9.5Ve 852 0
6 V* V479 Sct HXB 18 26 15.0561548880 -14 50 54.247274304 12.02 12.23 11.27 11.04   ON6V((f))z 613 2

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