Note: this is an
archived version which has been superseded. The current SNR
catalogue is at
http://www.mrao.cam.ac.uk/surveys/snrs/
G132.7+1.3
HB3
- Right Ascension: 02 17 40
- Declination: +62 45
- Size (/arcmin): 80
- Type: S
- Flux density at 1 GHz (/Jy): 45
- Spectral Index: 0.6
Notes: Has been called G132.4+2.2.
- Radio: Faint shell, adjacent to W3/4/5 complex.
- Optical: Complete, filamentary shell, shock excited spectra.
- X-ray: Partial shell.
- Point sources: Pulsar nearby.
- Distance: Interaction with surroundings suggests 2.2 kpc.
References:
- van den Bergh et al. 1973, ApJS, 26, 19. Optical.
- Velusamy & Kundu 1974, A&A, 32, 375. NRAO 300-ft at 2.7 GHz (5': S=33.8±7.0 Jy).
- d'Odorico & Sabbadin 1977, A&AS, 28, 439. Optical spectra.
ADS
- Read 1981, MNRAS, 194, 863. 6C at 151 MHz (4'.4) and HMT at 1.4 GHz (2') showing HI shell.
ADS
- Lozinskaya 1981, SvAL, 7, 17. Mean optical velocity.
ADS
- Fesen & Gull 1983, PASP, 95, 196. Optical image.
ADS
- Leahy et al. 1985, ApJ, 294, 183. IPC observations.
ADS
- Landecker et al. 1987, AJ, 94, 111. DRAO at 408 MHz (3'.5×4': S=75±15 Jy), plus review of flux densities.
ADS
- Routledge et al. 1991, A&A, 247, 529. DRAO at 1.4 GHz (1'.0×1'.1) for HI, plus CO observations.
ADS
- Fesen et al. 1995, AJ, 110, 2876. Optical imaging and spectroscopy, DRAO at 408 MHz (3'.5×4') and 1.4 GHz (1'.0×1'.1).
ADS
- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA detection of compact OH emission.
ADS
Last updated: 1 Aug 2000
Dave Green/MRAO, Cambridge, UK/D.A.Green@mrao.cam.ac.uk