G27.8+0.6
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- Right Ascension: 18 39 50
- Declination: −04 24
- Size (/arcmin): 50×30
- Type: F
- Flux density at 1 GHz (/Jy): 30
- Spectral Index: varies
- Radio: Filled-centre, with spectral turnover.
- X-ray: Possible pulsar wind nebula.
- Distance: Optical extinction suggests 4.0 kpc.
References:
- Reich et al. 1984, A&A, 133, L4. Effelsberg 100-m at 2.7 GHz (4.′3: S=23±2 Jy), and 4.75 GHz (2.′4: S=18±2 Jy) and NRO 45-m at 10.2 GHz (smoothed to 4.′3: S=8.5±2 Jy).
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- Frail et al. 1996, AJ, 111, 1651. OH emission near remnant.
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- Biggs & Lyne 1996, MNRAS, 282, 691. Pulsar search.
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- Casandjian & Grenier 2008, A&A, 489, 849. γ-ray observations.
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- Misanovic et al. 2010, ApJ, 725, 931. XMM-Newton pulsar/wind nebula search.
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- Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.′5: S=21.0±1.1 Jy) including polarisation and review of flux densities.
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- Froebrich et al. 2015, MNRAS, 454, 2586. H2 IR observations.
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- Lee et al. 2019, AJ, 157, 123. [FeII] and H2 IR observations.
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- Wang et al. 2020, A&A, 639, A72. Optical extinction for distance.
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Last updated: 14 Dec 2022
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