G353.6-0.7

Note: this is an archived version which has been superseded. The current SNR catalogue is at https://www.mrao.cam.ac.uk/surveys/snrs/

Notes: Has erroneously been called G353.6−0.37.

Radio: Shell, brighter to S.
X-ray: Patchy shell, brighter to E.
Point sources: Central X-ray source.
Distance: Various observations suggest 3.2 kpc, optical extinction suggests 3.5 kpc.

References:

Tian et al. 2008, ApJ, 679, L85. SGPS at 1.4 GHz (100''), plus 843 MHz (43'') and X-ray observations. ADS
Halpern & Gotthelf 2010, ApJ, 710, 941. XMM-Newton observations. ADS
Tian et al. 2010, ApJ, 712, 790. XMM-Newton, Suzaku and CO observations. ADS
H.E.S.S. Collaboration: Abramowski et al. 2011, A&A, 531, A81. H.E.S.S. observations. ADS
Bamba et al. 2012, ApJ, 756, 149. Suzaku observations. ADS
also see: Bamba et al. 2012, ApJ, 761, 80. Erratum. ADS
Klochkov et al. 2013, A&A, 556, A41. XMM-Newton and other X-ray observations. ADS
Fukuda et al. 2014, ApJ, 788, 94. H.E.S.S., SGPS HI and CO observations. ADS
Nayana et al. 2017, MNRAS, 467, 155. GMRT at 325 MHz (97''×135'') and 610 MHz (105''×150''), plus other observations. ADS
de Wilt et al. 2017, MNRAS, 468, 2093. Molecular line observations of region. ADS
Doroshenko et al. 2017, A&A, 608, A23. XMM-Newton observations. ADS
Condon et al. 2017, ApJ, 851, 100. Fermi observations. ADS
Guo et al. 2018, ApJ, 853, 2. Fermi observations. ADS
H.E.S.S. Collaboration: Abdalla et al. 2018, A&A, 612, A1. H.E.S.S. observations. ADS
Maxted et al. 2018, MNRAS, 474, 662. CO and HI observations. ADS
Cui et al. 2019, ApJ, 887, 47. Fermi observations. ADS
Wang et al. 2020, A&A, 639, A72. Optical extinction for distance. ADS

Last updated: 14 Dec 2022

Dave Green / Cambridge, UK /