Note: this is an archived version which has been superseded.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

G330.2+1.0 ADS: search fulltext or title/keyword/abstract

• Right Ascension: 16 01 06
• Declination: −51 34
• Size (/arcmin): 11
• Type: S?
• Flux density at 1 GHz (/Jy): 5?
• Spectral Index: 0.3

Radio: Clumpy non-thermal emission, possibly a distorted shell.

X-ray: Shell.

Point sources: Central compact X-ray source.

Distance: HI absorption indicates >4.9 kpc.

References:

• Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=8.6 Jy) and Parkes 64-m at 5 GHz (4': S=4.0 Jy). ADS
• Caswell et al. 1983, MNRAS, 204, 915. FIRST at 1415 MHz (47''×52''), and MOST at 843 MHz (43''×55''). ADS
• Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×55'': S=4.7 Jy). ADS
• Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations. ADS
• McClure-Griffiths et al. 2001, ApJ, 551, 394. ATCA and Parkes 64-m at 1.4 GHz (1.'8×2.'0), plus HI. ADS
• Torii et al. 2006, PASJ, 58, L11. ASCA detection. ADS
• Park et al. 2009, ApJ, 695, 431. XMM-Newton and Chandra observations. ADS
• H.E.S.S. Collaboration: Abramowski et al. 2014, MNRAS, 441, 790. H.E.S.S. upper limit. ADS
• Doroshenko et al. 2018, A&A, 618, A76. XMM-Newton observations of central source. ADS
• Williams et al. 2018, ApJ, 855, 118. XMM-Newton observations. ADS
• Borkowski et al. 2018, ApJ, 868, L21. Chandra observations for expansion study. ADS
• Mayer & Becker 2021, A&A, 651, A40. Multi-epoch Chandra observations for proper motion of compact source. ADS

Last updated: 15 Dec 2022

home | documentation | detailed listings | summary listings

Dave Green / Cambridge, UK /