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Supernova of AD 1181 and its Remnant: 3C 58

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Handbook of Supernovae
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Abstract

Every year astronomers see hundreds of supernova explosions in other galaxies, but in our own galaxy, the Milky Way, those have been rare events, only five over the last 1000 years. One of the more mysterious events happened back in AD 1181 and was discovered by Chinese and Japanese astronomers as a “guest star” in the constellation Cassiopeia. Today this guest star is known to us as supernova SN 1181. This historical supernova explosion most likely left behind the synchrotron nebula 3C 58 (supernova remnant G130.7+3.1), a nebula produced by the wind of a fast-spinning neutron star, the pulsar J 0205+6449. 3C 58 is very similar to the Crab Nebula in age, distance, size, and morphology, but much less luminous. Like the Crab Nebula, 3C 58 also does not show a shell-type remnant that would indicate the interaction of the supernova shock wave with the ambient medium. Here, I review what we know about SN 1181 and 3C 58 and the probable connection between them.

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References

  • Abdo AA et al (2009) Discovery of pulsations from the pulsar J0205+6449 in SNR 3C 58 with the fermi gamma-ray space telescope. Astrophys J 699:L102–L107

    Article  ADS  Google Scholar 

  • Aleksić J et al (2014) Discovery of TeV γ-ray emission from the pulsar wind nebula 3C 58 by MAGIC. Astron Astrophys 567:L8

    Article  ADS  Google Scholar 

  • Aller HD, Reynolds SP (1985) Evolution of the centimeter flux of 3C58 and the Crab Nebula. In: Kafatos MC, Henry RBC (eds) The Crab Nebula and related supernova remnants. Cambridge University Press, Cambridge/New York, pp 75–78

    Google Scholar 

  • Arnett WD, Bahcall JN, Kirshner RP, Woosley SE (1989) Supernova 1987A. Ann Rev Astron Astrophys 27:629–700

    Article  ADS  Google Scholar 

  • Artyukh VS, Dagkesamanskii VV, Vitkevich RD, Kozhukhov VN (1969) Flux densities and spectral indices for the sources in the 3C and 3CR catalogs at 86-MHz frequency. Sov Astron 12:567

    ADS  Google Scholar 

  • Becker RH, Helfand DJ, Szymkowiak AE (1982) An X-ray study of two Crablike supernova remnants – 3C 58 and CTB 80. Astrophys J 255:557–563

    Article  ADS  Google Scholar 

  • Becker RH, White RL, Edwards AL (1991) A new catalog of 53,522 4.85 GHz sources. Astrophys J Suppl Ser 75:1–229

    Article  ADS  Google Scholar 

  • Begelman MC, Li ZY (1992) An axisymmetric magnetohydrodynamic model for the Crab pulsar wind bubble. Astrophys J 397:187–195

    Article  ADS  Google Scholar 

  • Bennett AS (1962) The revised 3C catalogue of radio sources. Mem R Astron Soc 68:163

    ADS  Google Scholar 

  • Bietenholz MF (2006) Radio images of 3C 58: expansion and motion of its wisp. Astrophys J 645:1180–1187

    Article  ADS  Google Scholar 

  • Bietenholz MF, Kassim NE, Weiler KW (2001) The radio spectral index and expansion of 3C 58. Astrophys J 560:772–778

    Article  ADS  Google Scholar 

  • Bietenholz MF, Kondratiev V, Ransom S, Slane P, Bartel N, Buchner S (2013) The proper motion of PSR J0205+6449 in 3C 58. Mon Not R Astron Soc 431:2590–2598

    Article  ADS  Google Scholar 

  • Bocchino F, Warwick RS, Marty P, Lumb D, Becker W, Pigot C (2001) The X-ray nebula of the filled center supernova remnant 3C 58 and its interaction with the environment. Astron Astrophys 369:1078–1087

    Article  ADS  Google Scholar 

  • Camilo F et al (2002) Discovery of radio pulsations from the x-ray pulsar J0205+6449 in supernova remnant 3C 58 with the Green Bank telescope. Astrophys J 571:L41–L44

    Article  ADS  Google Scholar 

  • Chevalier RA (2000) A Model for the x-ray luminosity of pulsar nebulae. Astrophys J 539:L45–L48

    Article  ADS  Google Scholar 

  • Chevalier RA (2004) Pulsar wind nebulae: theoretical aspects and observational constraints. Adv Space Res 33:456–460

    Article  ADS  Google Scholar 

  • Clark DH, Stephenson FR (1977) The historical supernovae, 1st edn. Pergamon Press, Oxford/New York

    Google Scholar 

  • Conway RG, Kellermann KI, Long RJ (1963) The radio frequency spectra of discrete radio sources. Mon Not R Astron Soc 125:261

    Article  ADS  Google Scholar 

  • Edge DO, Shakeshaft JR, McAdam WB, Baldwin JE, Archer S (1959) A survey of radio sources at a frequency of 159 Mc/s. Mem R Astron Soc 68:37–60

    ADS  Google Scholar 

  • Fanti C, Felli M, Ficarra A, Salter CJ, Tofani G, Tomasi P (1974) A 408 MHz fan-beam survey at low galactic latitudes. I. The observations and a catalogue of small diameter sources. Astron Astrophys Suppl Ser 16:43–61

    ADS  Google Scholar 

  • Fesen R, Rudie G, Hurford A, Soto A (2008) Optical Imaging and spectroscopy of the galactic supernova remnant 3C 58 (G130.7+3.1). Astrophys J Suppl Ser 174:379–395

    Article  ADS  Google Scholar 

  • Foster T, MacWilliams J (2006) Modeling the neutral hydrogen interstellar medium: a better kinematic distance tool. Astrophys J 644:214–228

    Article  ADS  Google Scholar 

  • Furst E, Reich W, Reich P, Reif K (1990) A radio continuum survey of the galactic plane at 11-CENTIMETER wavelength – part four – a list of 6483 small diameter sources. Astron Astrophys Suppl Ser 85:805

    ADS  Google Scholar 

  • Gaensler BM, Slane PO (2006) The evolution and structure of pulsar wind nebulae. Ann Rev Astron Astrophys 44:17–47. astro-ph/0601081

    Google Scholar 

  • Gotthelf EV (2004) A spin-down power threshold for pulsar wind nebula generation? In: Camilo F, Gaensler BM (eds) Young Neutron stars and their environments, IAU Symposium, vol 218. Astronomical Society of the Pacific, p 225. ISBN:1-58381-178-8

    Google Scholar 

  • Gotthelf EV, Helfand DJ, Newburgh L (2007) A shell of thermal x-ray emission surrounding the young crab-like remnant 3C 58. Astrophys J 654:267–272

    Article  ADS  Google Scholar 

  • Green DA (1986) Observations of 3C 58 at 151 and 2695 MHz. Mon Not R Astron Soc 218:533–540

    Article  ADS  Google Scholar 

  • Green DA (1987) Confirmation of 3C 58’s increasing radio flux density. Mon Not R Astron Soc 225:11P–15P

    Article  ADS  Google Scholar 

  • Green DA, Scheuer PAG (1992) Upper limits on the infrared flux density of the ‘filled-centre’ supernova remnant 3C58. Mon Not R Astron Soc 258:833–840

    Article  ADS  Google Scholar 

  • Green AJ, Baker JR, Landecker TL (1975) Observations of eight supernova remnants at 15 GHz. Astron Astrophys 44:187–194

    ADS  Google Scholar 

  • Hobbs G, Lorimer DR, Lyne AG, Kramer M (2005) A statistical study of 233 pulsar proper motions. Mon Not R Astron Soc 360:974–992

    Article  ADS  Google Scholar 

  • Horton PW, Conway RG, Daintree EJ (1969) Measurement of the spectrum of 387 radio sources at centimetre wavelengths-I. Mon Not R Astron Soc 143:245

    Article  ADS  Google Scholar 

  • Hurley-Walker N et al (2009) AMI observations of northern supernova remnants at 14–18 GHz. Mon Not R Astron Soc 396:365–376

    Article  ADS  Google Scholar 

  • Kellermann KI, Pauliny-Toth IIK, Williams PJS (1969) The spectra of radio sources in the revised 3c catalogue. Astrophys J 157:1

    Article  ADS  Google Scholar 

  • Kepler J (1606) Ioannis Kepleri … De Iesu Christi servatoris nostri vero anno quatuor annos in usitatam epocham desiderantis: (titulus currens: natalitio, consideratio novissimae sententiae Laurentii Suslygae …, Sylva chronologica). doi:10.3931/e-rara-1168

    Google Scholar 

  • Kothes R (2013) Distance and age of the pulsar wind nebula 3C 58. Astron Astrophys 560:A18

    Article  ADS  Google Scholar 

  • Kothes R, Fedotov K, Foster TJ, Uyanıker B (2006) A catalogue of Galactic supernova remnants from the Canadian Galactic plane survey. I. Flux densities, spectra, and polarization characteristics. Astron Astrophys 457:1081–1093

    Article  ADS  Google Scholar 

  • Kothes R, Landecker TL, Reich W, Safi-Harb S, Arzoumanian Z (2008) DA 495: an aging pulsar wind nebula. Astrophys J 687:516–531

    Article  ADS  Google Scholar 

  • Kothes R, Sun XH, Reich W, Foster TJ (2014) G141.2+5.0, a new pulsar wind nebula discovered in the cygnus arm of the milky way. Astrophys J 784:L26

    Google Scholar 

  • Kundu MR, Velusamy T (1972) Brightness and polarization structure of four supernova remnants 3C 58, IC 443, W28, and W44 at 2.8 centimeter wavelength. Astron Astrophys 20:237–244

    ADS  Google Scholar 

  • Landecker TL, Higgs LA, Wendker HJ (1993) G76.9+1.0, a supernova remnant and unusual properties. Astron Astrophys 276:522

    Google Scholar 

  • Langston G, Minter A, D’Addario L, Eberhardt K, Koski K, Zuber J (2000) The first galactic plane survey at 8.35 and 14.35 GHZ. Astron J 119:2801–2827

    Article  ADS  Google Scholar 

  • Livingstone MA, Ransom SM, Camilo F, Kaspi VM, Lyne AG, Kramer M, Stairs IH (2009) X-ray and radio timing of the pulsar in 3C 58. Astrophys J 706:1163–1173

    Article  ADS  Google Scholar 

  • Morsi HW, Reich W (1987) 32 GHz radio continuum observations of four plerionic supernova remnants. Astron Astrophys Suppl Ser 69:533–540

    ADS  Google Scholar 

  • Murray SS, Slane PO, Seward FD, Ransom SM, Gaensler BM (2002) Discovery of x-ray pulsations from the compact central source in the supernova remnant 3C 58. Astrophys J 568:226–231

    Article  ADS  Google Scholar 

  • Ng CY, Romani RW (2004) fitting pulsar wind Tori. Astrophys J 601:479–484

    Article  ADS  Google Scholar 

  • Ostriker JP, Gunn JE (1969) On the nature of pulsars. I. Theory. Astrophys J 157:1395

    Article  ADS  Google Scholar 

  • Pacini F (1967) Energy emission from a neutron star. Nature 216:567–568

    Article  ADS  Google Scholar 

  • Pacini F, Salvati M (1973) On the evolution of supernova remnants. Evolution of the magnetic field, particles, content, and luminosity. Astrophys J 186:249–266

    Article  ADS  Google Scholar 

  • Pauliny-Toth IIK, Wade CM, Heeschen DS (1966) Positions and flux densities of radio sources. Astrophys J Suppl Ser 13:65

    Article  ADS  Google Scholar 

  • Planck Collaboration et al (2014) Planck intermediate results. XXXI. Microwave survey of galactic supernova remnants. ArXiv e-prints 1409.5746

    Google Scholar 

  • Reich P, Reich W, Furst E (1997) The Effelsberg 21 CM radio continuum survey of the Galactic plane between L = 95.5 deg and L = 240 deg. Astron Astrophys Suppl Ser 126:413–435

    Article  ADS  Google Scholar 

  • Reich W, Fürst E, Kothes R (1998) High frequency observations of plerions and combined-type SNRs. Memorie della Società Astronomica Italiana 69:933

    ADS  Google Scholar 

  • Roger RS, Costain CH, Bridle AH (1973) The low-frequency spectra of nonthermal radio sources. Astron J 78:1030

    Article  ADS  Google Scholar 

  • Salter CJ, Reynolds SP, Hogg DE, Payne JM, Rhodes PJ (1989) 84 gigahertz observations of five Crab-like supernova remnants. Astrophys J 338:171–177

    Article  ADS  Google Scholar 

  • Sastry CV, Pauliny-Toth IIK, Kellermann KI (1967) Observations of the polarization of discrete radio sources at 6-cm wavelength. Astron J 72:230–234

    Article  ADS  Google Scholar 

  • Shakeshaft JR, Ryle M, Baldwin JE, Elsmore B, Thomson JH (1955) A survey of radio sources between declinations − 38 and + 83. Mem R Astron Soc 67:106

    ADS  Google Scholar 

  • Slane P, Helfand DJ, van der Swaluw E, Murray SS (2004) New constraints on the structure and evolution of the pulsar wind nebula 3C 58. Astrophys J 616:403–413

    Article  ADS  Google Scholar 

  • Slane P, Helfand DJ, Reynolds SP, Gaensler BM, Lemiere A, Wang Z (2008) The infrared detection of the pulsar wind nebula in the galactic supernova remnant 3C 58. Astrophys J 676:L33–L36

    Article  ADS  Google Scholar 

  • Slane PO, Helfand DJ, Murray SS (2002) New constraints on neutron star cooling from Chandra observations of 3C 58. Astrophys J 571:L45–L49

    Article  ADS  Google Scholar 

  • Stephenson FR (1971) Suspected supernova in A.D. 1181. Q J R Astron Soc 12:10

    Google Scholar 

  • Stephenson FR, Green DA (2002) Historical supernovae and their remnants. In: Stephenson FR, Green DA (eds) Historical supernovae and their remnants. International series in astronomy and astrophysics, vol 5. Clarendon Press, Oxford. ISBN:0198507666 5

    Google Scholar 

  • Sun XH, Reich P, Reich W, Xiao L, Gao XY, Han JL (2011) A Sino-German λ6 cm polarization survey of the galactic plane. VII. Small supernova remnants. Astron Astrophys 536:A83

    Google Scholar 

  • Taylor AR et al (2003) The Canadian Galactic Plane Survey. Astron J 125:3145–3164

    Article  ADS  Google Scholar 

  • Torii K, Slane PO, Kinugasa K, Hashimotodani K, Tsunemi H (2000) ASCA observations of the crab-like supernova remnant 3C 58. Publ Astron Soc Jpn 52:875–885

    Article  ADS  Google Scholar 

  • van der Swaluw E (2003) Interaction of a magnetized pulsar wind with its surroundings. MHD simulations of pulsar wind nebulae. Astron Astrophys 404:939–947

    Article  ADS  Google Scholar 

  • Wallace BJ, Landecker TL, Taylor AR (1994) H I voids around filled-center supernova remnants. Astron Astrophys 286:565–578

    ADS  Google Scholar 

  • Weiler KW, Panagia N (1978) Are crab-type supernova remnants (plerions) short-lived? Astron Astrophy 70:419

    ADS  Google Scholar 

  • Williams PJS, Kenderdine S, Baldwin JE (1966) A survey of radio sources and background radiation at 38 Mc/s. Mem R Astron Soc 70:53–110

    ADS  Google Scholar 

  • Wilson AS, Weiler KW (1976) The brightness and polarization structure of the suspected supernova remnant 3 C 58 at centimetre wavelengths. Astron Astrophys 49:357–374

    ADS  Google Scholar 

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Acknowledgements

I would like to express my special thanks to Dave Green for making a new finding chart for the guest star of AD 1181 for me. I also would like to express my deepest appreciation to Michael Bietenholz (radio), Rob Fesen (optical), and Pat Slane (X-ray) for providing their beautiful maps for this publication. I would also like to thank Tom Landecker for careful reading of this document. The Dominion Radio Astrophysical Observatory is a national facility operated by the National Research Council Canada.

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Kothes, R. (2016). Supernova of AD 1181 and its Remnant: 3C 58. In: Alsabti, A., Murdin, P. (eds) Handbook of Supernovae. Springer, Cham. https://doi.org/10.1007/978-3-319-20794-0_47-1

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  • DOI: https://doi.org/10.1007/978-3-319-20794-0_47-1

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