Note: this is
an archived version which has been superseded. The current SNR
catalogue is at
https://www.mrao.cam.ac.uk/surveys/snrs/
G28.6−0.1
ADS: search fulltext or
title/keyword/abstract
- Right Ascension: 18 43 55
- Declination: −03 53
- Size (/arcmin): 13×9
- Type: S
- Flux density at 1 GHz (/Jy): 3?
- Spectral Index: ?
- Radio: Poorly defined regions of non-thermal emission.
- X-ray: Diffuse shell, with thermal and non-thermal emission.
- Point sources: Pulsar in NE.
- Distance: HI absorption and CO suggests 9.6 kpc.
References:
- Helfand et al. 1989, ApJ, 341, 151. VLA at 1.4 GHz (15'') and 5 GHz (15'').
ADS
- Bamba et al. 2001, PASJ, 53, L21. ASCA observations.
ADS
- Ueno et al. 2003, ApJ, 588, 338. Chandra observations.
ADS
- Ebisawa et al. 2005, ApJ, 635, 214. Chandra observations.
ADS
- Zyuzin et al. 2018, MNRAS, 476, 2177. Pulsar observations.
ADS
- Ranasinghe & Leahy 2018, MNRAS, 477, 2243. VGPS HI absorption, plus CO observations.
ADS
- Lee et al. 2019, AJ, 157, 123. [FeII] IR observations.
ADS
- Devin et al. 2021, A&A, 647, A68. Fermi observations.
ADS
- Dokara et al. 2021, A&A, 651, A86. VLA at 4 to 8 GHz (18'': S=1.2 Jy) including polarisation, and Spitzer observations.
ADS
- Castelletti et al. 2021, A&A, 653, A62.VLA 74-MHz survey flux density, and other low-frequency radio flux densities.
ADS
- Sofue et al. 2021, ApJS, 253, 17. Nobeyama 45-m CO observations (20'') of region.
ADS
Last updated: 20 Dec 2022
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