G119.5+10.2
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CTA 1
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- Right Ascension: 00 06 40
- Declination: +72 45
- Size (/arcmin): 90?
- Type: S
- Flux density at 1 GHz (/Jy): 36
- Spectral Index: 0.6
Notes: Has been called G119.5+10.3.
- Radio: Incomplete shell, with ‘breakout’ to NW.
- Optical: Faint diffuse nebulosities.
- X-ray: Centrally brightened.
- Point sources: Central pulsar.
- Distance: Associated HI shell indicates 1.4 kpc.
References:
- Sieber et al. 1979, A&A, 74, 361. Effelsberg 100-m at 2.7 GHz (4.′4: S=23.6±2.8 Jy).
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- Sieber et al. 1981, A&A, 103, 393. Effelsberg 100-m at 2.7 GHz and 1.7 GHz (7.′6: S=31.6±2.5 Jy), and 151 MHz (4′: S=62.6±6 Jy).
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- Fesen et al. 1981, ApJ, 247, 148. Optical, including spectra.
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- Fesen et al. 1983, ApJS, 51, 337. Deep [OIII] imagery.
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- Seward 1990, ApJS, 73, 781. Einstein observations.
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- Simonetti 1992, ApJ, 386, 170. VLA observations of background sources for rotation measure studies.
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- Pineault et al. 1993, AJ, 105, 1060. DRAO at 1.4 GHz (1′: S=34±4 Jy), plus HI and IRAS.
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- Seward et al. 1995, ApJ, 453, 284. ROSAT observations.
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- Biggs & Lyne 1996, MNRAS, 282, 691. Pulsar search.
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- Slane et al. 1997, ApJ, 485, 221. ASCA and ROSAT observations.
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- Pineault et al. 1997, A&A, 324, 1152. DRAO at 408 MHz (3.′5) and 1.4 GHz (1.′0).
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- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
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- Brazier et al. 1998, MNRAS, 295, 819. Studies of central, compact γ-ray source.
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- Mavromatakis et al. 2000, A&A, 353, 371. Optical imagery.
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- Roberts et al. 2001, ApJS, 133, 451. ASCA observations.
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- Reich 2002, in NSPS, p1. Effelsberg 100-m at 1.4 GHz (9.′4).
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- Slane et al. 2004, ApJ, 601, 1045. XMM-Newton observations of central source.
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- Halpern et al. 2004, ApJ, 612, 398. Chandra observations of central nebula, plus optical and radio limits for compact source.
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- Casandjian & Grenier 2008, A&A, 489, 849. γ-ray observations.
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- Abdo et al. 2008, Science, 322, 1218. Fermi detection of pulsar.
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- Lin et al. 2010, ApJ, 725, L1. XMM-Newton observations of pulsar.
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- Caraveo et al. 2010, ApJ, 725, L6. XMM-Newton observations of pulsar.
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- Sun et al. 2011, A&A, 535, A64. Urumqi 25-m at 4.8 GHz (9.′5: S=11.6±1.2 Jy) and Effelsberg 100-m at 2.6 GHz (4.′4: S=20.3±2.0 Jy) including polarisation.
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- Lin et al. 2012, MNRAS, 426, 2283. Suzaku observations.
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- Mignani et al. 2013, MNRAS, 430, 1354. Optical limits for pulsar.
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- Aliu et al. 2013, ApJ, 764, 38. γ-ray observations.
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- Li et al. 2016, ApJ, 831, 19. Fermi observations of pulsar.
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- Ackermann et al. 2018, ApJS, 237, 32. Fermi observations.
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Last updated: 9 Apr 2019
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