G41.1−0.3 ADS: search title/keyword/abstract or fulltext

3C397 ADS: search title/keyword/abstract or fulltext

• Right Ascension: 19 07 34
• Declination: +07 08
• Size (/arcmin): 4.5×2.5
• Type: S
• Flux density at 1 GHz (/Jy): 25
• Spectral Index: 0.50

Radio: 3C397 is two sources: the E is the SNR, the W is a HII region.

X-ray: Brighter to the E and W, with central component.

Distance: HI absorption suggest 8.5 kpc.

References:

• Kundu et al. 1974, AJ, 79, 132. NRAO 140-ft at 10 GHz (3′) and 5 GHz (6′). ADS
• Velusamy & Kundu 1974, A&A, 32, 375. NRAO 300-ft at 2.7 GHz (5′: S=21.3±1.2 Jy for both components). ADS
• Caswell et al. 1975, A&A, 45, 239. HI absorption. ADS
• Dickel & DeNoyer 1975, AJ, 80, 437. Arecibo S_430 MHz=82±51 Jy, also Algonquin 46-m at 10.6 GHz (3′: S=12±2 Jy), and Haystack 36-m at 15.5 GHz (2.′3: S=8.5±3.0 Jy). ADS
• Caswell et al. 1975, AuJPA, 37, 39. Molonglo at 408 MHz (3′: S=29.8 Jy) and Parkes 64-m at 5 GHz (4′: S=8.7 Jy). ADS
• Altenhoff et al. 1979, A&AS, 35, 23. Effelsberg 100-m at 4.9 GHz (2.′6). ADS
• Caswell et al. 1982, MNRAS, 200, 1143. FIRST at 1.4 GHz (52″×58″). ADS
• Becker et al. 1985, ApJ, 296, 461. VLA at 1.4 and 5 GHz (8″), plus Einstein observations. ADS
• Morsi & Reich 1987, A&AS, 71, 189. Effelsberg 100-m at 32 GHz (smoothed to 30″: S=4.10±0.19 Jy). ADS
• Kassim 1992, AJ, 103, 943. VLA at 327 MHz (3.′5×3.′6: S=46.3 Jy). ADS
• Anderson & Rudnick 1993, ApJ, 408, 514. VLA at 1.45 and 4.89 GHz, for spectral index studies. ADS
• Gorham et al. 1996, ApJ, 458, 257. Pulsar search. ADS
• Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations. ADS
• Chen et al. 1999, ApJ, 520, 737. ASCA and ROSAT observations. ADS
• Dyer & Reynolds 1999, ApJ, 526, 365. VLA at 1.5 GHz (6.″6×6.″9) and 4.8 GHz (5.″6×6.″4), including polarisation and comparison with ROSAT image. ADS
• Safi-Harb et al. 2000, ApJ, 545, 922. ROSAT, ASCA and other X-ray observations. ADS
• Sugizaki et al. 2001, ApJS, 134, 77. ASCA survey observations. ADS
• Aharonian et al. 2001, A&A, 375, 1008. H.E.S.S. limit. ADS
• Safi-Harb et al. 2005, ApJ, 618, 321. Chandra observations. ADS
• Reach et al. 2006, AJ, 131, 1479. Spitzer observations. ADS
• Jiang et al. 2010, ApJ, 712, 1147. CO observations of region. ADS
• Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.′5: S=18.5±1.1 Jy) including polarisation and review of flux densities. ADS
• Yang et al. 2013, ApJ, 766, 44. Suzaku spectroscopy. ADS
• Yamaguchi et al. 2015, ApJ, 801, L31. Suzaku observations. ADS
• Clark et al. 2015, ApJ, 809, L2. Fermi observations. ADS
• Kilpatrick et al. 2016, ApJ, 816, 1. CO observations, including broad lines. ADS
• Leahy & Ranasinghe 2016, ApJ, 817, 74. VGPS for HI absorption. ADS
• Koo et al. 2016, ApJ, 821, 20. Spitzer and Herschel flux densities (and comparison with X-ray properties). ADS
• Ranasinghe & Leahy 2018, AJ, 155, 204. VGPS HI absorption observations. ADS
• Lee et al. 2019, AJ, 157, 123. [FeII] IR observations. ADS
• Dokara et al. 2021, A&A, 651, A86. VLA at 4 to 8 GHz (18″: S=1.3 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
• Ohshiro et al. 2021, ApJ, 913, L34. XMM-Newton observations. ADS
• Sofue et al. 2021, ApJS, 253, 17. Nobeyama 45-m CO observations (20″) of region. ADS
• Ergin et al. 2021, MNRAS, 501, 4226. Fermi limit. ADS
• Shanahan et al. 2022, ApJ, 939, 92. VLA at 1 to 2 GHz, including polarisation. ADS

Last updated: 5 Jan 2024

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