Note: this is
an archived version which has been superseded. The current SNR
catalogue is at
https://www.mrao.cam.ac.uk/surveys/snrs/
G69.0+2.7
ADS: search fulltext or
title/keyword/abstract
CTB 80
- Right Ascension: 19 53 20
- Declination: +32 55
- Size (/arcmin): 80?
- Type: ?
- Flux density at 1 GHz (/Jy): 120?
- Spectral Index: varies
Notes: An association with a SN in AD1408 has been suggested. Has been called G68.8+2.8.
- Radio: Compact core, flat spectrum plateau, and steeper spectrum extensions, with spectral break?
- Optical: Expanding nebulosity near centre, with filaments to the SW and far NE.
- X-ray: Diffuse emission with compact source.
- Point sources: Pulsar at W edge of core.
- Distance: HI observations suggest 1.5 kpc, and optical absorption suggests 4.6 kpc.
References:
- Angerhofer et al. 1981, A&A, 94, 313. WSRT at 610 MHz (56''×103'') 1.4 GHz (24''×44'') and 5 GHz (7''×13''), plus optical.
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- Becker et al. 1982, ApJ, 255, 557. X-ray observations.
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- Sofue et al. 1983, PASJ, 35, 437. NRO 45-m at 10.2 GHz (2.'7).
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- Velusamy & Kundu 1983, JApA, 4, 253. VLA of compact sources.
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- Blair et al. 1984, ApJ, 282, 161. Optical images and spectra.
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- Wang & Seward 1984, ApJ, 285, 607. Einstein observations.
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- Strom et al. 1984, A&A, 139, 43. Radio observations of flat spectrum component, VLA 5 GHz (1.''7) and 1.4 GHz.
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- Mantovani et al. 1985, A&A, 145, 50. Bologna at 408 MHz (2.'6×4.'9: S=67.5±10.5 Jy), Effelsberg 100-m at 1.41 (9': S=62±9 Jy), 1.72 (7.'6: S=66±5 Jy), 2.7 (4.'5: S=52±4 Jy) and 4.75 GHz (2.'4: S=44±3.3 Jy), plus review of flux densities.
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- Kulkarni et al. 1988, Nature, 331, 50. Pulsar detection.
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- Angelini et al. 1988, ApJ, 330, L43. EXOSAT spectra.
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- Fesen et al. 1988, Nature, 334, 229. IRAS of surrounding shell.
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- Junkes et al. 1988, LNP, 316, 134. Effelsberg 100-m at 2.7 GHz (4.'3), including polarisation.
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- Whitehead et al. 1989, MNRAS, 237, 1109. Optical of core.
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- Salter et al. 1989, ApJ, 338, 171. NRAO 12-m at 84.2 GHz of core, plus review of flux densities.
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- Hester & Kulkarni 1989, ApJ, 340, 362. Optical imaging and spectroscopy.
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- Koo et al. 1990, ApJ, 364, 178. Large, expanding HI shell.
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- Greidanus & Strom 1990, A&A, 240, 376. Optical kinematics of core.
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- Koo et al. 1993, ApJ, 417, 196. VLA at 1.4 GHz of surrounding HI (1'), plus IRAS.
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- Safi-Harb et al. 1995, ApJ, 439, 722. ROSAT observations.
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- Srinivasan 1997, ApJ, 489, 170. γ-ray observations of pulsar.
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- Mavromatakis et al. 2001, A&A, 371, 300. Optical observations.
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- Butler et al. 2002, A&A, 395, 845. HST detection of pulsar.
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- Migliazzo et al. 2002, ApJ, 567, L141. Pulsar proper motion study.
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- Castelletti et al. 2003, AJ, 126, 2114. GMRT at 240 and 618 MHz (17''×26'' and 6''×10'') and VLA at 324 and 1380 MHz (63''×73'' and 78''×93'').
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- Moon et al. 2004, ApJ, 610, L33. Chandra and HST observations of core.
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- Li et al. 2005, ApJ, 628, 931. Chandra observations of pulsar and surroundings.
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- Golden et al. 2005, ApJ, 635, L153. High resolution radio observations of pulsar and surroundings.
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- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3': S=72±7 Jy) and 1420 MHz (~1': S=56±5 Jy), including polarisation and review of flux densities.
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- Kang & Koo 2007, ApJS, 173, 85. SGPS of high velocity HI.
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- Albert et al. 2007, ApJ, 669, 1143. γ-ray observations.
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- Zeiger et al. 2008, ApJ, 674, 271. Proper motion of pulsar.
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- Gao et al. 2011, A&A, 529, A159. Urumqi 25-m at 5 GHz (9.'5: S=36±4 Jy), including polarisation and review of flux densities.
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- Leahy & Ranasinghe 2012, MNRAS, 423, 718. CGPS at 1.4 GHz, including HI, plus ROSAT observations.
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- Park et al. 2013, ApJ, 777, 14. Arecibo of HI in region.
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- Planck Collaboration: Arnaud et al. 2016, A&A, 586, A134. Planck flux densities at 30 and 44 GHz.
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- Shan et al. 2018, ApJS, 238, 35. Optical absorption for distance.
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- Li et al. 2020, RAA, 20, 186. Radio study from various surveys.
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- Araya & Herrera 2021, MNRAS, 502, 472. Fermi observations.
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Last updated: 16 Dec 2022
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