G54.4−0.3
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(HC40)
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- Right Ascension: 19 33 20
- Declination: +18 56
- Size (/arcmin): 40
- Type: S
- Flux density at 1 GHz (/Jy): 28
- Spectral Index: 0.5
Notes: Has been called G54.5−0.3.
- Radio: Shell, in complex region.
- Optical: Faint filaments.
- Point sources: Pulsar outside NW rim.
- Distance: HI and CO observations suggest 6.6 kpc, H2 emission suggests 5.4 kpc, optical extinction suggests 6.6 kpc.
References:
- Velusamy & Kundu 1974, A&A, 32, 375. NRAO 300-ft at 2.7 GHz (5′: S=34.4±5.0 Jy).
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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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- Caswell 1985, AJ, 90, 1224. DRAO at 1.4 GHz (1.′3×2.′6: S=18±4 Jy).
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- Velusamy et al. 1986, JApA, 7, 105. WSRT at 609 MHz (50″×191″ smoothed to 100″×200″).
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- Junkes et al. 1992, A&AS, 96, 1. Surrounding CO.
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- Junkes et al. 1992, A&A, 261, 289. Nearby IRAS sources.
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- Boumis et al. 2005, A&A, 443, 175. Optical observations.
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- Reach et al. 2006, AJ, 131, 1479. Spitzer observations.
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- Kang & Koo 2007, ApJS, 173, 85. High velocity HI.
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- Andersen et al. 2011, ApJ, 742, 7. Spitzer observations.
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- Park et al. 2013, ApJ, 777, 14. Arecibo of HI in region.
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- Froebrich et al. 2015, MNRAS, 454, 2586. H2 IR observations.
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- Karpova et al. 2017, MNRAS, 466, 1757. X-ray observations of pulsar.
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- Ranasinghe & Leahy 2017, ApJ, 843, 119. HI and CO observations.
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- Lee et al. 2019, AJ, 157, 123. H2 IR observations.
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- Chawner et al. 2020, MNRAS, 493, 2706. Herschel observations.
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- Lee et al. 2020, AJ, 160, 263. H2 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=0.6 Jy) including polarisation, and Spitzer observations.
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Last updated: 20 Dec 2022
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