2023PASJ...75.1273Y


Query : 2023PASJ...75.1273Y

2023PASJ...75.1273Y - Publ. Astron. Soc. Jap., 75, 1273-1279 (2023/December-0)

Spectral analysis of the Galactic supernova remnant Kesteven 69 with Suzaku.

YAMAUCHI S. and PANNUTI T.G.

Abstract (from CDS):

The results of a Suzaku observation of the supernova remnant (SNR) Kesteven 69 = G21.8-0.6 are presented. To estimate the sky background precisely, we conducted a simultaneous fit of the source region spectrum with the background region spectrum and found that the SNR spectrum is well represented by a two-component ionizing plasma model composed of a low-temperature plasma at kTe = 0.80 ± 0.11 keV and a high-temperature plasma at kTe = 1.5 ± 0.4 keV. The existence of a low-ionized Fe K line at 6.49 ± 0.07 keV was confirmed. The center energy of the line is consistent with those of type Ia SNRs.

Abstract Copyright: © The Author(s) 2023. Published by Oxford University Press on behalf of the Astronomical Society of Japan.

Journal keyword(s): ISM: individual objects (G21.8-0.6, Kes 69) - ISM: supernova remnants - X-rays: ISM

Simbad objects: 11

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Number of rows : 11
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 IC 433 G 05 40 31.3524514488 -11 39 56.022239160   14       ~ 34 0
2 SNR G272.2-03.2 SNR 09 06 50 -52 07.0           SNIa 78 0
3 SNR G337.2-00.7 SNR 16 39 15.0 -47 48 27           ~ 68 1
4 SNR G352.7-00.1 SNR 17 27 43 -35 06.5           ~ 79 1
5 SNR G006.4-00.1 SNR 18 00 31.2011719 -23 25 48.001099           ~ 782 1
6 XMMU J183234.3-100434 X 18 32 34.3 -10 04 34           ~ 2 1
7 XMMU J183236.4-101146 X 18 32 36.4 -10 11 46           ~ 2 1
8 SNR G021.8-00.6 SNR 18 32 45 -10 08.0           ~ 137 0
9 SWIFT J183251.6-100104 CV* 18 32 51.3999688713 -10 01 07.066413270       21.57   ~ 9 2
10 SNR G041.1-00.3 SNR 19 07 22.6 +07 10 44           ~ 252 2
11 NAME Galactic Ridge ? ~ ~           ~ 543 1

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