G126.2+1.6    

• Right Ascension: 01 22 00
• Declination: +64 15
• Size (/arcmin): 70
• Type: S?
• Flux density at 1 GHz (/Jy): 6
• Spectral Index: 0.5

Radio: Poorly defined shell.

Optical: Filaments, mostly in W.

References:

• Reich et al. 1979, A&A, 78, L13. Effelsberg 100-m at 1.4 GHz (9': S=6.8±0.7 Jy) and 2.7 GHz (4'.4: S=3.9±0.4 Jy). ADS
• Blair et al. 1980, ApJ, 242, 592. Optical detection and spectra. ADS
• Rosado 1982, RMxAA, 5, 127. Optical spectra. ADS
• Fesen et al. 1983, ApJS, 51, 337. Deep [OIII] imagery. ADS
• Fürst et al. 1984, A&A, 133, 11. Effelsberg 100-m at 2.7 GHz (4'.4) and 4.8 GHz (2'.6). ADS
• Joncas et al. 1989, A&A, 219, 303. DRAO at 408 MHz (3'.5×3'.9: S=12±2.5 Jy) and part at 1.4 GHz (1'.1×1'.0), plus review of flux densities. ADS
• Xilouris et al. 1993, A&A, 270, 393. Optical imaging. ADS
• Lorimer et al. 1998, A&A, 331, 1002. Pulsar search. ADS
• Reich et al. 2003, A&A, 408, 961. Effelsberg 100-m at 863 MHz (14'.5: S=6.1±1.6 Jy). ADS
• Boumis et al. 2005, A&A, 443, 175. Optical observations. ADS
• Tian & Leahy 2006, A&A, 447, 205. CGPS at 408 MHz (3'.4×3'.8: S=9.7±3.9 Jy) and 1.4 GHz (1'.0×1'.1: S=6.7±2.1 Jy), plus other observations for spectral index studies. ADS
• Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=5.7±0.7 Jy) and 1420 MHz (~1': S=6.4±1.1 Jy), including review of flux densities. ADS
• Sun et al. 2007, A&A, 463, 993. Urumqi 25-m at 5 GHz (9'.5: S=2.6±0.6 Jy), including polarisation. ADS
   also see: Sun et al. 2007, A&A, 469, 1003. Erratum. ADS

Last updated: 20 Feb 2009