G12.8−0.0
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- Right Ascension: 18 13 37
- Declination: −17 49
- Size (/arcmin): 3
- Type: C?
- Flux density at 1 GHz (/Jy): 0.8
- Spectral Index: 0.5
Notes: Has been called G12.7+0.0, G12.82−0.02, G12.83−0.02.
- Radio: Shell.
- X-ray: Diffuse.
- Point sources: Central X-ray pulsar.
References:
- Brogan et al. 2005, ApJ, 629, L105. VLA at 330 MHz (19″×32″), plus other observations.
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- Ubertini et al. 2005, ApJ, 629, L109. INTEGRAL and other observations.
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- Aharonian et al. 2006, ApJ, 636, 777. H.E.S.S. detection.
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- Albert et al. 2006, ApJ, 637, L41. γ-ray observations.
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- Brogan et al. 2006, ApJ, 639, L25. VLA at 330 MHz (42″: S=1.2±0.1 Jy), plus other observations.
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- Landi et al. 2006, ApJ, 651, 190. X-ray observations.
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- Funk et al. 2007, A&A, 470, 249. XMM-Newton observations, CO observations of surroundings.
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- Helfand et al. 2007, ApJ, 665, 1297. Chandra observations.
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- Hewitt & Yusef-Zadeh 2009, ApJ, 694, L16. OH maser search.
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- Gotthelf & Halpern 2009, ApJ, 700, L158. Pulsar detection.
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- Halpern et al. 2012, ApJ, 753, L14. Pulsar observations.
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- Araya et al. 2018, ApJ, 859, 69. Fermi observations.
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- Dzib et al. 2018, ApJ, 866, 100. VLA of central source.
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- Ho et al. 2020, MNRAS, 498, 4396. Chandra and other X-ray observations, for proper motions of pulsar.
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- Dokara et al. 2021, A&A, 651, A86. VLA at 4 to 8 GHz (18″) including polarisation, and Spitzer observations.
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- Camilo et al. 2021, ApJ, 917, 67. Radio detection of pulsar.
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- Dzib & Rodríguez 2021, ApJ, 923, 228. Pulsar proper motion.
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Last updated: 20 Dec 2022
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