Skip to main content

Thank you for visiting nature.com. You are using a browser version with limited support for CSS. To obtain the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles and JavaScript.

  • Letter
  • Published:

Unusual radio arcs discovered in the radio source G318.9+0.4

Abstract

THE radio source G318.9 + 0.4 has been tentatively identified as a supernova remnant (SNR)1,2. Here I report observations at 843 MHz revealing a remarkable network of arcs in the object which exclude it from any of the standard classes of SNRs. The arcs outline an approximately elliptical region enclosing a bright off-centre core component which has several curved extensions. Although the appearance of the arc structures is unprecedented, G318.9 + 0.4 might belong to a recently proposed class of non-thermal axisymmetric radio sources unrelated to SNRs3. Alternatively, the core component may indeed be a SNR, excited by the stellar remnant of the supernova event, with the arc emission arising through jet activity.

This is a preview of subscription content, access via your institution

Access options

Buy this article

Prices may be subject to local taxes which are calculated during checkout

Similar content being viewed by others

References

  1. Caswell, J. L. & Haynes, R. F. Astr. Astrophys. 171, 261–276 (1987).

    ADS  CAS  Google Scholar 

  2. Broadbent, A., Haslam, C. G. T. & Osborne, J. L. Mon. Not. R. astr. Soc. 237, 381–410 (1989).

    Article  ADS  CAS  Google Scholar 

  3. Becker, R. H. & Helfand, D. J. Nature 313, 115–118 (1985).

    Article  ADS  Google Scholar 

  4. Mills, B. Y. Proc. astr. Soc. Aust. 4, 156–159 (1981).

    Article  ADS  Google Scholar 

  5. Whiteoak, J. B. Z., Large, M. I., Cram, L. E. & Piestrzynski, B. Proc. astr. Soc. Aust. 8, 176–179 (1989).

    Article  ADS  Google Scholar 

  6. Haynes, R. F., Caswell, J. L. & Simons, L. W. J. Aust J. Phys. Astrophys. Suppl. 45, 1–87 (1978).

    ADS  Google Scholar 

  7. Georgelin, Y. P. & Georgelin, Y. M. Astr. Astrophys. Suppl. Ser. 3, 1–49 (1970).

    ADS  Google Scholar 

  8. Lyngâ, G. & Hansson, N. Astr. Astrophys. Suppl. Ser. 6, 327–414 (1972).

    ADS  Google Scholar 

  9. Shaver, P. A. & Goss, W. M. Aust J. Phys. Astrophys. Suppl. 14, 133–196 (1970).

    ADS  Google Scholar 

  10. Shaver, P. A. Astr. Astrophys. 105, 306–312 (1982).

    ADS  Google Scholar 

  11. Green, D. A. Astrophys. Space Sci. 148, 3–74 (1988).

    Article  ADS  CAS  Google Scholar 

  12. Velusamy, T., Kundu, M. R. & Becker, R. H. Astr. Astrophys 51, 21–24 (1976).

    ADS  Google Scholar 

  13. Clifton, T. R. et al. IAU Circ. 4422 (1987).

  14. Kulkarni, S. R. et al. Nature 331, 50–53 (1988).

    Article  ADS  Google Scholar 

  15. Manchester, R. N. Astr. Astrophys. 171, 205–215 (1987).

    ADS  CAS  Google Scholar 

  16. Helfand, D. J. & Becker, R. H. Nature 313, 118–119 (1985).

    Article  ADS  Google Scholar 

  17. Hjellming, R. M. & Johnston, K. J. Proc. lAU Symp. 97 (eds Heeschen, D. S. & Wade, C. M.) 197–204 (Reldel, Dordrecht, 1981).

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Whiteoak, J. Unusual radio arcs discovered in the radio source G318.9+0.4. Nature 347, 157–158 (1990). https://doi.org/10.1038/347157a0

Download citation

  • Received:

  • Accepted:

  • Issue Date:

  • DOI: https://doi.org/10.1038/347157a0

Comments

By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.

Search

Quick links

Nature Briefing

Sign up for the Nature Briefing newsletter — what matters in science, free to your inbox daily.

Get the most important science stories of the day, free in your inbox. Sign up for Nature Briefing