Abstract
We report here a search for periodic emission of X rays from MXB1730–335 (the Rapid Burster, which is the most unusual X-ray burst source1 out of about 30 other bursters) during the long flat top bursts2. Two events from the 63 bursts showed clear peaks in the frequency power spectra at ∼0.5 s in period. However, this is unlikely to be a pulsar period, because the periods of these two bursts are different.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Kunieda, H. et al. Publ. astr. Soc. Japan (in the press).
Inoue, H. et al. Nature 283, 358 (1980).
Lewin, W. H. G. et al. Astrophys. J. Lett. 207, L95 (1976).
Cordova, F. A., Chester, T. J., Tuohy, I. R. & Garmire, G. P. Astrophys. J. 235, 163 (1980).
Patterson, J. Astrophys. J. Suppl. 45, 517 (1981).
Van Horn, H. M., Wesemael, F. & Winget, D. E. Astrophys. J. Lett. 235, L143 (1980).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Tawara, Y., Hayakawa, S., Kunieda, H. et al. Discovery of 0.5-s oscillations in long flat top bursts from the Rapid Burster. Nature 299, 38–41 (1982). https://doi.org/10.1038/299038a0
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1038/299038a0
This article is cited by
-
Astron observations of the Rapid Burster MXB 1730-335 and constraints on burster parameters from spectra of trailing bursts
Astrophysics and Space Science (1990)
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.