Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-05T03:34:36.321Z Has data issue: false hasContentIssue false
  • English
  • Français

Observational Aspects of Supernova Remnants

Published online by Cambridge University Press:  14 August 2015

B. Y. Mills
B. Y. Mills*
Affiliation:
University of Sydney, Sydney, Australia

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A supernova event may lead to four observable features: a pulsar, an expanding nebulosity, a radio source and an X-ray source. The great majority of supernovae do not produce observable pulsars, and discussion is restricted largely to the other features. An increasing number of X-ray sources is now being detected and the structure and spectrum of the stronger sources investigated; these observations yield information about the physical state of the remnant. Recently, 11 new optical and radio remnants have been found in the Magellanic Clouds. These have led to a good determination of the Σ – D relation, thus providing a more reliable distance scale for galactic SNR, but have also shown that a one-to-one correspondence between a radio source and a supernova event is questionable. When these remnants are combined with corrected earlier catalogues and a new southern catalogue containing a high proportion of distant old remnants the number of known SNR is about 150. The evolution of galactic SNR may be investigated empirically, and although the derived rate of occurrence is very uncertain a rate of about 2 supernovae per century is consistent with most determinations. The galactic SNR are distributed rather like the radio disc emission, but more closely confined to the galactic plane, and selected SNR show evidence of a spiral pattern.

Type
Part 3: Supernova Remnants
Information
Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 311 - 327
Copyright
Copyright © Reidel 1974 

References

Bergh, S. van den: 1971, Astrophys. J. 165, 457.Google Scholar
Bergh, S. van den, Marscher, A. P., and Terzian, Y.: 1973, Astrophys. J. Suppl. 26, 19.CrossRefGoogle Scholar
Berkhuijsen, E. M.: 1973, Astron. Astrophys. 24, 143.Google Scholar
Blandford, R. D., Ostriker, P. J., Paccini, F., and Rees, M. J.: 1973, Astron. Astrophys. 23, 145.Google Scholar
Broten, N. W.: 1972, Australian J. Phys. 25, 599.Google Scholar
Bunner, A. N., Colemand, P. L., Kraushaar, W. L., and McCammon, D.: 1972, Astrophys. J. Letters 172, L67.CrossRefGoogle Scholar
Burginyon, G., Hill, R., Seward, F., Tarter, B., and Toor, A.: 1973b, Astrophys. J. Letters 180, L75.Google Scholar
Burginyon, G., Hill, R., Palmieri, T., Scudder, J., Seward, F., Stoering, J., and Toor, A.: 1973a, Astrophys. J. 179, 615.Google Scholar
Byrne, P. B. and Butler, C. J.: 1973, Nature Phys. Sci. 244, 6.Google Scholar
Cameron, A. G. W.: 1970, Ann. Rev. Astron. Astrophys. 8, 179.Google Scholar
Caswell, J. L.: 1972, Australian J. Phys. 25, 443.Google Scholar
Caswell, J. L. and Goss, W. M.: 1970, Astrophys. Letters 7, 142.Google Scholar
Clark, D. H., Caswell, J. L., and Green, A. J.: 1973, Nature 246, 28.Google Scholar
Clarke, J. N.: 1971, Proc. Astron. Soc. Australia 2, 44.Google Scholar
Combe, V. and Large, M. I.: 1973, Astrophys. Letters 14, 59.Google Scholar
Davies, J. G., Lyne, A. G., and Seirdakis, J. H.: 1972, Nature 20, 229.CrossRefGoogle Scholar
Detre, L.: 1970, IAU Circ. No. 2269.Google Scholar
Dickel, J. R. and Milne, D. K.: 1972, Australian J. Phys. 25, 539.CrossRefGoogle Scholar
Dickel, J. R., Milne, D. K., Kerr, A. R., and Ables, J. G.: 1973, Australian J. Phys. 26, 379.Google Scholar
Downes, D.: 1971, Astron. J. 76, 305.Google Scholar
Downs, G. S. and Thompson, A. R.: 1972, Astron. J. 77, 120.Google Scholar
Dulk, G. A. and Slee, O. B.: 1972, Australian J. Phys. 25, 429.Google Scholar
Fabian, A. C., Zarnecki, J. C., and Culhane, J. L.: 1973, The Soft X-ray Structure of Cassiopeia A, preprint.Google Scholar
Findlay, J. W.: 1972, Astrophys. J. 174, 527.Google Scholar
Giacconi, R., Murray, S., Gursky, H., and Kellogg, E.: 1972, Astrophys. J. 178, 281.Google Scholar
Goss, W. M., Allen, R. J., Ekers, R. D., and Bruyn, A. G. de: 1973, Nature Phys. Sci. 243, 42.Google Scholar
Gottesman, S. T., Broderick, J. J., Brown, R. L., Balick, B., and Palmer, P.: 1972, Astrophys. J. 174, 383.Google Scholar
Ilovaisky, S. A. and Lequeux, J.: 1972a, Astron. Astrophys. 18, 169.Google Scholar
Ilovaisky, S. A. and Lequeux, J.: 1972b, Astron. Astrophys. 20, 347.Google Scholar
Katgert, P. and Oort, J. H.: 1967, Bull. Astron. Inst. Neth. 19, 239.Google Scholar
Kerr, F. J.: 1970, in Becker, W. and Contopoulos, G. (eds.), ‘The Spiral Structure of Our Galaxy’, IAU Symp. 38, 95.Google Scholar
Kundu, M. R. and Becker, R. H.: 1972, Astron. J. 77, 459.Google Scholar
Kundu, M. R. and Velusamy, T.: 1972, Astron. Astrophys. 20, 237.Google Scholar
Large, M. I. and Vaughan, A. E.: 1972, Nature Phys. Sci. 236, 117.Google Scholar
Le Marne, A. E.: 1968, Monthly Notices Roy. Astron. Soc. 139, 461.Google Scholar
Lozinskaya, T. A.: 1972, Soviet Astron. 20, 219.Google Scholar
McGee, R. X. and Newton, L. M.: 1972, Australian J. Phys. 25, 619.Google Scholar
McGee, R. X., Brooks, J. W., and Batchelor, R. A.: 1972a, Australian J. Phys. 25, 581.Google Scholar
McGee, R. X., Brooks, J. W., and Batchelor, R. A.: 1972b, Australian J. Phys. 25, 613.Google Scholar
Mathewson, D. S. and Clarke, J. N.: 1972, Astrophys. J. Letters 178, L105.Google Scholar
Mathewson, D. S. and Clarke, J. N.: 1973a, Astrophys. J. 179, 89.Google Scholar
Mathewson, D. S. and Clarke, J. N.: 1973b, Astrophys. J. 180, 725.Google Scholar
Mathewson, D. S. and Clarke, J. N.: 1973c, Astrophys. J. 182, 697.Google Scholar
Mathewson, D. S. and Healey, J. R.: 1964, in Kerr, F. J. and Rodgers, A. W. (eds.), ‘The Galaxy and the Magellanic Clouds’, IAU Symp. 20, 283.Google Scholar
Mills, B. Y.: 1971, 12th International Conference on Cosmic Rays, Invited and Rapporteur Papers, p. 72.Google Scholar
Mills, B. Y. and Aller, L. H.: 1971, Australian J. Phys. 24, 609.Google Scholar
Milne, D. K.: 1970, Australian J. Phys. 23, 425.Google Scholar
Milne, D. K.: 1970, in Davies, R. D. and Smith, F. G. (eds.), ‘The Crab Nebula’, IAU Symp. 46, 248.Google Scholar
Milne, D. K.: 1972a, Australian J. Phys. 25, 307.Google Scholar
Milne, D. K.: 1972b, Astrophys. Letters 11, 167.Google Scholar
Minkowski, R.: 1958, Rev. Mod. Phys. 30, 1048.CrossRefGoogle Scholar
Minkowski, R.: 1959, in Bracewell, R. N. (ed.), ‘Paris Symposium on Radio Astronomy’, IAU Symp. 9, 315.Google Scholar
Moffat, P. H.: 1971, Monthly Notices Roy. Astron. Soc. 153, 401.Google Scholar
Palmieri, T. M., Burginyon, G. A., Hill, R. W., Scudder, J. K., and Seward, F. D.: 1972, Astrophys. J. 177, 387.Google Scholar
Reichley, P. E., Downs, G. S., and Morris, G. A.: 1970, Astrophys. J. Letters 159, L35.Google Scholar
Schwartz, D. A., Bleach, R. D., Boldt, E. A., Holt, S. S., and Serlemitsos, P. J.: 1972, Astrophys. J. Letters 173, L51.CrossRefGoogle Scholar
Schwartz, D. A., Bleach, R. D., Boldt, E. A., Holt, S. S., and Serlemitsos, P. J.: 1972, Rep. NASA-TM-X-65825, NASA, Greenbelt, Maryland.Google Scholar
Schönhardt, R. E.: 1973, Nature Phys. Sci. 243, 62.Google Scholar
Searle, L.: 1971, Astrophys. J. 168, 327.Google Scholar
Shaver, P. A.: 1969, Observatory 89, 227.Google Scholar
Shklovskii, I. S.: 1962, Soviet Astron. 6, 162.Google Scholar
Stevens, J. C. and Garmire, G. P.: 1973, Astrophys. J. Letters 180, L19.Google Scholar
Tammann, G. A.: 1970, in Becker, W. and Contopoulos, G. (eds.), ‘The Spiral Structure of Our Galaxy’, IAU Symp. 38, 236.Google Scholar
Tsarevsky, G. S.: 1973, Astrophys. Letters 10, 71.Google Scholar
Tucker, W. H.: 1971, Science 172, 372.Google Scholar
Velusamy, T. and Kundu, M. R.: 1973, Polarization of Supernova Remnants: Internal Faraday Effects and Derived Magnetic Fields, preprint.Google Scholar
Westerlund, B. E. and Mathewson, D. S.: 1966, Monthly Notices Roy. Astron. Soc. 131, 371.CrossRefGoogle Scholar
Willis, A. G.: 1972, Ph.D. Thesis, University of Illinois.Google Scholar
Woltjer, L.: 1972, Ann. Rev. Astron. Astrophys. 10, 129.Google Scholar
Zarnecki, J. C., Culhane, J. L., Fabian, A. C., Rapley, C. G., Silk, R., Parkinson, J. H., and Pounds, K. A.: 1973, A Low Energy X-Ray Map of the Puppis-A Supernova Remnants, preprint.Google Scholar