G74.9+1.2
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CTB 87
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- Right Ascension: 20 16 02
- Declination: +37 12
- Size (/arcmin): 8×6
- Type: F
- Flux density at 1 GHz (/Jy): 9
- Spectral Index: 0.3
- Radio: Filled-centre, with high polarisation, and larger faint halo,
- X-ray: Centrally brightened.
- Point sources: Compact X-ray source in SE.
- Distance: Optical extinction gives 6.1 kpc.
References:
- Dickel & DeNoyer 1975, AJ, 80, 437. Arecibo S430 MHz=12.2±9.7 Jy, S318 MHz=17.7±5.0 Jy.
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- Weiler & Shaver 1978, A&A, 70, 389. WSRT at 610 MHz (57″×94″: S=9.1±1.2 Jy), 1.4 (24″×40″: S=8.7±1.2 Jy) and 5 GHz (24″×40″: S=5.6±1.3 Jy).
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- Geldzahler et al. 1980, A&A, 84, 237. Effelsberg 100-m at 2.7 GHz (4.′4: S=7.6±0.5 Jy).
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- Wilson 1980, ApJ, 241, L19. Einstein observations.
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- van Gorkom et al. 1982, MNRAS, 198, 757. WSRT HI absorption of nearby compact source.
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- Seaquist & Gilmore 1982, AJ, 87, 378. VLA observations of nearby source.
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- Morsi & Reich 1987, A&AS, 69, 533. Effelsberg 100-m at 32 GHz (smoothed to 40″: S=1.47±0.19 Jy).
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- Green & Gull 1989, MNRAS, 237, 555. VLA at 1.4 GHz (1.′2×1.′4) including HI.
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- Salter et al. 1989, ApJ, 338, 171. NRAO 12-m at 84.2 GHz, plus review of flux densities.
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- Pineault & Chastenay 1990, MNRAS, 246, 169. DRAO at 408 MHz (3.′4×5.′8: S=11.6±0.4 Jy) and 1.4 GHz (1.′0×1.′7: S=7.2±0.3 Jy).
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- Asaoka & Koyama 1990, PASJ, 42, 625. Ginga X-ray spectrum.
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- Wendker et al. 1991, A&A, 241, 551. DRAO at 408 MHz (3.′5×5.′2: S=13.3±0.8 Jy) and Effelsberg 100-m at 4.8 GHz (S=7.5±0.7 Jy).
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- Wallace et al. 1994, A&A, 286, 565. HI of surroundings.
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- Cho et al. 1994, AJ, 108, 634. CO of adjacent molecular clouds.
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- Gorham et al. 1996, ApJ, 458, 257. Pulsar search.
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- Biggs & Lyne 1996, MNRAS, 282, 691. Pulsar search.
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- Wallace et al. 1997, A&A, 317, 212. DRAO at 408 MHz (3.′4×5.′5) and 1.4 GHz (1.′0×1.′6) including HI (smoothed to 2′).
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- Lorimer et al. 1998, A&A, 331, 1002. Pulsar search.
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- Kothes et al. 2003, ApJ, 588, 852. CGPS at 1.4 GHz (1′×1.′6) including HI, plus CO observations.
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- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3′: S=11.9±0.9 Jy) and 1420 MHz (~1′: S=7.1±1.1 Jy), including polarisation and review of flux densities.
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- Hurley-Walker et al. 2009, MNRAS, 396, 365. Radio observations at 14 to 18 GHz.
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- Sitnik 2010, ARep, 54, 317. Hα and CO observations of region.
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- Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.′5: S=6.4±0.4 Jy) including polarisation and review of flux densities.
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- Matheson et al. 2013, ApJ, 774, 33. Chandra observations.
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- Bassani et al. 2014, A&A, 561, A108. X-ray and γ-ray observations.
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- Aliu et al. 2014, ApJ, 788, 78. γ-ray detection.
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- Saha 2016, MNRAS, 460, 3563. Fermi observations.
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- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
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- Liu et al. 2018, ApJ, 859, 173. CO observations.
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- Abeysekara et al. 2018, ApJ, 861, 134. γ-ray observations.
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- Guest et al. 2020, MNRAS, 491, 3013. XMM-Newton observations.
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- Kothes et al. 2020, MNRAS, 496, 723. Effelsberg 100-m at 4.75 (2.′5), 10.55 (1.′2), 14.7 (0.′85) and 32 GHz (0.′45), plus other radio survey observations.
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- Reich et al. 2022, A&A, 668, A39. Effelsberg 100-m at 14.7 (51″: S=4.3±0.4 Jy) and 17.3 GHz (43″: S=3.9±0.3 Jy), plus review of radio spectrum.
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Last updated: 4 Jan 2024
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