G160.9+2.6
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HB9
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- Right Ascension: 05 01 00
- Declination: +46 40
- Size (/arcmin): 140×120
- Type: S
- Flux density at 1 GHz (/Jy): 110
- Spectral Index: 0.64
Notes: Has been called G160.5+2.8 and G160.4+2.8.
- Radio: Large, filamentary shell.
- Optical: Incomplete shell.
- X-ray: Centrally brightened.
- Point sources: Pulsar within boundary of the remnant, plus several nearby compact radio sources.
- Distance: Various observations suggests less than 4 kpc, optical extinction suggests 0.5 kpc.
References:
- D′Odorico & Sabbadin 1977, A&AS, 28, 439. Optical spectra.
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- Damashek et al. 1978, ApJ, 225, L31. Pulsar.
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- Lozinskaya 1981, SvAL, 7, 17. Mean optical velocity.
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- Dwarakanath et al. 1982, JApA, 3, 207. Radio observations at 34.5 MHz (26′×40′: S=750±150 Jy), plus review of flux densities.
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- van Gorkom et al. 1982, MNRAS, 198, 757. WSRT HI absorption to nearby point source.
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- Seaquist & Gilmore 1982, AJ, 87, 378. VLA observations of nearby source.
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- Leahy 1987, ApJ, 322, 917. Einstein observations.
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- Leahy & Roger 1991, AJ, 101, 1033. DRAO at 408 MHz (3.′5×4.′8) and 1.4 GHz (1.′0×1.′4), including HI and discussion of distance.
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- Yamauchi & Koyama 1993, PASJ, 45, 545. Hard X-ray observations.
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- Leahy & Aschenbach 1995, A&A, 293, 853. ROSAT observations.
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- Biggs & Lyne 1996, MNRAS, 282, 691. Pulsar search.
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- Leahy et al. 1998, A&A, 339, 601. 232 MHz (3.′8×5.′2), 151 MHz (4.′2×5.′8) and Effelsberg 100-m at 4.7 GHz (2.′5) for spectral index studies.
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- Roger et al. 1999, A&AS, 137, 7. 22 MHz flux density (S=1130±340 Jy).
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- Reich et al. 2003, A&A, 408, 961. Effelsberg 100-m at 863 MHz (14.′5: S=91±3 Jy).
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- Fürst & Reich 2004, in MIM, p141. Effelsberg 100-m at 1.4 and 2.7 GHz (9.′3), including polarisation.
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- Kaplan et al. 2006, ApJS, 163, 344. X-ray upper limit on compact sources.
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- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3′: S=102±7 Jy) and 1420 MHz (~1′: S=54.0±2.9 Jy), including polarisation and review of flux densities.
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- Leahy & Tian 2007, A&A, 461, 1013. CGPS at 408 MHz (2.′8×3.′9: S=117.8±5.3 Jy) and 1.4 GHz (58″×80″: S=65.9±3.4 Jy).
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- Gao et al. 2011, A&A, 529, A159. Urumqi 25-m at 5 GHz (9.′5: S=34±3 Jy), including polarisation and review of flux densities.
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- Gosachinskii 2013, AstL, 39, 179. HI observations of region.
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- Araya et al. 2014, MNRAS, 444, 860. Fermi detection.
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- Tung et al. 2017, AJ, 154, 156. CGPS at 408 MHz (2.′8×3.′5).
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- Sezer et al. 2019, MNRAS, 489, 4300. Suzaku observations.
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- Zhao et al. 2020, ApJ, 891, 137. Optical extinction for distance.
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- Saito et al. 2020, PASJ, 72, 65. Suzaku observations.
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- Oka & Ishizaki 2022, PASJ, 74, 625. Fermi observations.
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- Jing et al. 2023, MNRAS, 523, 4949. FAST observations of pulsar, for distance.
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Last updated: 18 Mar 2024
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