G40.5−0.5 ADS: search fulltext or title/keyword/abstract

• Right Ascension: 19 07 10
• Declination: +06 31
• Size (/arcmin): 22
• Type: S
• Flux density at 1 GHz (/Jy): 11
• Spectral Index: 0.4

Radio: Shell, brightest to the NE.

Point sources: Central pulsar.

Distance: Optical extinction suggests 5.1 kpc.

References:

• Altenhoff et al. 1979, A&AS, 35, 23. Effelsberg 100-m at 4.9 GHz (2.'6). ADS
• Downes et al. 1980, A&A, 92, 47. Effelsberg 100-m at 1.7 GHz (7.'6: S=9.3±1.3 Jy), and 2.7 GHz (4.'4: S=7.2±0.5 Jy), plus review of flux densities. ADS
• Aharonian et al. 2001, A&A, 375, 1008. H.E.S.S. limit. ADS
• Yang et al. 2006, ChJAA, 6, 210. CO observations of surroundings. ADS
• Abdo et al. 2007, ApJ, 664, L91. γ-ray observations. ADS
• Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.'5: S=6.4±0.3 Jy) including polarisation and review of flux densities. ADS
• Aliu et al. 2014, ApJ, 787, 166. γ-ray observations of region. ADS
• Lyne et al. 2017, ApJ, 834, 137. Pulsar detection. ADS
• Duvidovich et al. 2020, MNRAS, 491, 5732. VLA at 1.5 GHz (39.''5×51.''1), and CO observations of part. ADS
• Wang et al. 2020, A&A, 639, A72. Optical extinction for distance. ADS
• Dokara et al. 2021, A&A, 651, A86. VLA at 4 to 8 GHz (18'': S=0.05 Jy) including polarisation, and Spitzer observations. ADS
• Li et al. 2021, ApJ, 913, L33. Fermi observations of region. ADS
• Sofue et al. 2021, ApJS, 253, 17. Nobeyama 45-m CO observations (20'') of region. ADS
• Crestan et al. 2021, MNRAS, 505, 2309. Fermi observations of region. ADS

Last updated: 20 Dec 2022

home | documentation | detailed listings | summary listings

Dave Green / Cambridge, UK /