G24.7+0.6
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- Right Ascension: 18 34 10
- Declination: −07 05
- Size (/arcmin): 30×15
- Type: C?
- Flux density at 1 GHz (/Jy): 20?
- Spectral Index: 0.2?
- Radio: Filled-centre, with faint shell, and a compact HII region to the S.
- Distance: Optical extinction suggests 2.7 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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- Reich et al. 1984, A&A, 133, L4. Effelsberg 100-m at 2.7 GHz (4.′3: S=19±3 Jy) and 4.75 GHz (2.′4: S=17±4 Jy) and NRO 45-m at 10.2 GHz (2.′7: S=15±3 Jy).
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- Becker & Helfand 1987, ApJ, 316, 660. VLA at 1.4 GHz (12″), and X-ray upper limit.
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- Biggs & Lyne 1996, MNRAS, 282, 691. Pulsar search.
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- Froebrich et al. 2015, MNRAS, 454, 2586. H2 IR observations.
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- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
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- Lee et al. 2019, AJ, 157, 123. H2 IR observations.
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- MAGIC Collaboration, Acciari et al. 2019, MNRAS, 483, 4578. γ-ray 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=0.9 Jy) including polarisation, and Spitzer observations.
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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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