G130.7+3.1
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3C58,
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SN1181
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- Right Ascension: 02 05 41
- Declination: +64 49
- Size (/arcmin): 9×5
- Type: F
- Flux density at 1 GHz (/Jy): 33
- Spectral Index: 0.07
Notes: This is the remnant of the SN of AD1181.
- Radio: Filled-centre, highly polarised, with high frequency turnover.
- Optical: Faint filaments.
- X-ray: Centrally brightened, with faint jet.
- Point sources: Central pulsar.
- Distance: HI absorption indicates 2 kpc.
References:
- Green et al. 1975, A&A, 44, 187. Effelsberg 100-m at 15.0 GHz (58″: S=26.7±0.5 Jy).
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- Wilson & Weiler 1976, A&A, 49, 357. WSRT at 610 MHz (58″×64″), 1.4 GHz (24″×27″) and 5 GHz (7″×8″).
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- van den Bergh 1978, ApJ, 220, L9. Optical observations.
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- Becker et al. 1982, ApJ, 255, 557. X-ray observations.
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- Green & Gull 1982, Nature, 299, 606. HI absorption distance.
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- Fesen 1983, ApJ, 270, L53. Optical spectra.
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- Reynolds & Aller 1985, AJ, 90, 2312. VLA at 1.4 GHz (2′), for limits of shell.
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- Davelaar et al. 1986, ApJ, 300, L59. EXOSAT spectrum.
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- Green 1986, MNRAS, 218, 533. 151 MHz observations (1.′2×1.′3: S=36±4 Jy), plus 2.7 GHz (4″), plus Einstein observations for limit on shell.
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- Green 1987, MNRAS, 225, 11P. Flux density increase at 408 MHz.
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- Morsi & Reich 1987, A&AS, 69, 533. Effelsberg 100-m at 32 GHz (26.″5: S=24.2±1.4 Jy).
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- Reynolds & Aller 1988, ApJ, 327, 845. VLA at 1.4 (2.″4) and 4.9 GHz (2.″5).
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- Salter et al. 1989, ApJ, 338, 171. NRAO 12-m at 84.2 GHz (90″: S=15.0±2.0 Jy), plus review of flux densities.
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- Asaoka & Koyama 1990, PASJ, 42, 625. Ginga X-ray spectrum.
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- Green & Scheuer 1992, MNRAS, 258, 833. IRAS upper limits.
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- Roberts et al. 1993, A&A, 274, 427. HI absorption.
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- Wallace et al. 1994, A&A, 286, 565. HI of surroundings.
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- Helfand et al. 1995, ApJ, 453, 741. ROSAT observations.
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- Torii et al. 2000, PASJ, 52, 875. ASCA observations.
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- Bietenholz et al. 2001, ApJ, 560, 772. VLA at 74 MHz (26″: S=33.6 Jy) and 327 MHz (8.″2: S=33.9 Jy), for spectral index and expansion studies.
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- Bocchino et al. 2001, A&A, 369, 1078. XMM-Newton observations.
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- Murray et al. 2002, ApJ, 568, 226. Chandra pulsar detection.
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- Camilo et al. 2002, ApJ, 571, L41. Pulsar detection in radio.
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- Reich 2002, in NSPS, p1. Effelsberg 100-m at 32 GHz (26″) for polarised intensity.
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- Slane et al. 2002, ApJ, 571, L45. Chandra observations.
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- Slane et al. 2004, ApJ, 616, 403. Deep Chandra imaging.
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- Bietenholz 2006, ApJ, 645, 1180. VLA at 1.4 GHz (1.″36) for expansion studies.
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- Kothes et al. 2006, A&A, 457, 1081. CGPS at 408 MHz (~3′: S=32.2±2.0 Jy) and 1420 MHz (~1′: S=31.9±1.0 Jy), including polarisation and review of flux densities.
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- Gotthelf et al. 2007, ApJ, 654, 267. XMM-Newton observations.
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- Slane et al. 2008, ApJ, 676, L33. Spitzer and other IR observations.
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- Fesen et al. 2008, ApJS, 174, 379. Optical observations for proper motion studies.
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- Shearer & Neustroev 2008, MNRAS, 390, 235. Optical observations of pulsar nebula.
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- Shibanov et al. 2008, A&A, 486, 273. Optical observations of pulsar nebula.
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- Abdo et al. 2009, ApJ, 699, L102. Fermi observations of pulsar.
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- Livingstone et al. 2009, ApJ, 706, 1163. Pulsar observations.
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- Hurley-Walker et al. 2009, MNRAS, 396, 365. Radio observations at 14 to 18 GHz.
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- Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.′5: S=31.7±3.0 Jy) including polarisation and review of flux densities.
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- Bietenholz et al. 2013, MNRAS, 431, 2590. Proper motion study of pulsar.
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- Kothes et al. 2013, A&A, 560, A18. CGPS HI observations for distance.
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- Aleksić et al. 2014, A&A, 567, L8. γ-ray detection.
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- Planck Collaboration: Arnaud et al. 2016, A&A, 586, A134. Planck flux densities at 7 frequencies between 30 and 353 GHz.
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- Guest & Safi-Harb 2020, MNRAS, 498, 821. Chandra observations.
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- Castelletti et al. 2021, A&A, 653, A62.VLA 74-MHz survey flux density.
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- Millard et al. 2021, ApJS, 257, 36. ISO far-IR spectroscopy.
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Last updated: 15 Dec 2022
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