G23.3−0.3
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W41
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- Right Ascension: 18 34 45
- Declination: −08 48
- Size (/arcmin): 27
- Type: S
- Flux density at 1 GHz (/Jy): 70
- Spectral Index: 0.5
- Radio: Distorted ring, in complex region, overlapping G22.7−0.2.
- X-ray: Possible extended emission, with compact sources.
- Point sources: Pulsar association suggested.
- Distance: HI and CO observations suggest 4.2 or 4.8 kpc, optical extinction suggests 3.4 kpc.
References:
- Shaver & Goss 1970, AuJPA, 14, 133. Molonglo at 408 MHz (3′) and Parkes 64-m at 5 GHz (4′).
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- Altenhoff et al. 1979, A&AS, 35, 23. Effelsberg 100-m at 4.9 GHz (2.′6).
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- Kassim 1992, AJ, 103, 943. VLA at 327 MHz (3.′3×3.′4: S=138 Jy).
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- Gaensler & Johnston 1995, MNRAS, 275, L73. Possible pulsar association.
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- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
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- Aharonian et al. 2005, Science, 307, 1938. H.E.S.S. detection.
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- Reach et al. 2006, AJ, 131, 1479. Spitzer possible detection.
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- Aharonian et al. 2006, ApJ, 636, 777. H.E.S.S. observations.
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- Albert et al. 2006, ApJ, 643, L53. γ-ray observations.
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- Landi et al. 2006, ApJ, 651, 190. X-ray observations.
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- Tian et al. 2007, ApJ, 657, L25. VGPS at 1.4 GHz (1′) including HI, plus XMM-Newton observations.
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- Leahy & Tian 2008, AJ, 135, 167. VGPS at 1.4 GHz (1′) including HI, plus CO observations.
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- Mukherjee et al. 2009, ApJ, 691, 1707. XMM-Newton and SWIFT observations.
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- Frail et al. 2013, ApJ, 773, L19. OH observations.
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- Castro et al. 2013, ApJ, 774, 36. Fermi observations.
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- H.E.S.S. Collaboration: Abramowski et al. 2015, A&A, 574, A27. H.E.S.S. observations.
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- Su et al. 2015, ApJ, 811, 134. CO observations of region.
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- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
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- Ranasinghe & Leahy 2018, AJ, 155, 204. VGPS HI absorption observations.
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- Lee et al. 2019, AJ, 157, 123. [FeII] IR observations.
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- Wang et al. 2020, A&A, 639, A72. Optical extinction for distance.
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- Dokara et al. 2021, A&A, 651, A86. VLA at 4 to 8 GHz (18″: S=1.8 Jy) including polarisation, and Spitzer observations.
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- Castelletti et al. 2021, A&A, 653, A62.VLA 74-MHz survey flux density, and other low-frequency radio flux densities.
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- Sofue et al. 2021, ApJS, 253, 17. Nobeyama 45-m CO observations (20″) of region.
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Last updated: 20 Dec 2022
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