2023RAA....23j5001Z


Query : 2023RAA....23j5001Z

2023RAA....23j5001Z - Research in Astron. and astroph., 23, part no 10, 5001 (2023/October-0)

Multi-wavelength Study of HESS J1303-631 with 14 yr of Fermi-LAT Data.

ZHOU L.-C., XIA Q., TIAN S.-T., GONG Y.-L. and FANG J.

Abstract (from CDS):

HESS J1303-631 is an extended TeV pulsar wind nebula powered by the pulsar PSR J1301-6305 detected with the High Energy Stereoscopic System. We present an analysis of the GeV γ-ray region of HESS J1303-631 with about 14 yr of Fermi Large Area Telescope data. The GeV γ-ray emission, coincident with the very-high-energy source, has a photon index of 1.69 ± 0.09 in 10-500 GeV band, and the GeV morphology has an extension to the same direction as indicated in the TeV band. Moreover, the observed multi-wavelength spectral energy distribution of the nebula is studied with a one-zone time-dependent leptonic model, in which the electrons/positrons injected into the nebula are assumed to have a broken power-law spectrum. The result indicates that the multi-wavelength non-thermal emission can be well reproduced via synchrotron radiation and inverse Compton scattering of the particles.

Abstract Copyright: © 2023. National Astronomical Observatories

Journal keyword(s): ISM: supernova remnants - radiation mechanisms: non-thermal - ISM: general

Simbad objects: 9

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Number of rows : 9
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 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
2 PSR J1301-6305 Psr 13 02 47.9992676 -63 10 48.001099           ~ 139 2
3 SNR G304.4-00.2 SN? 13 04 31.1 -63 02 08           ~ 3 0
4 3FGL J1305.7-6241 gam 13 05 35.1 -62 41 38           ~ 13 0
5 SNR G304.6+00.1 SNR 13 05 59 -62 42.0           ~ 93 0
6 PSR J1357-6429 Psr 13 57 02.525 -64 29 29.89           ~ 171 1
7 SNR G338.3-00.0 SNR 16 40 43.2 -46 31 48           ~ 175 2
8 PSR B1823-13 Psr 18 26 13.06 -13 34 48.1           ~ 460 1
9 ARGO J1907+0627 gam 19 08 12.24 +06 23 30.8           ~ 94 0

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