Abstract
IYENGAR et al.1 have reported observations of hard X rays from Her X-1, which seem to set an upper limit of 10% on the pulsating component in the energy range 20 to 45 keV. I offer a simple explanation that does not require the additional source of X rays postulated by Iyengar et al.
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
Rent or buy this article
Get just this article for as long as you need it
$39.95
Prices may be subject to local taxes which are calculated during checkout
References
Iyengar, V. S., Manchanda, R. K., Durgaprasad, N., Gokhale, G. S., Kunte, P. K., and Sreekantan, B. V., Nature, 251, 292–294 (1974).
Canute, V., Lodenquai, J., and Ruderman, M., Phys. Rev. D., 3, 2303–2308 (1971).
Pringle, J. E., and Rees, M. J., Astr. Astrophys., 21, 1–9 (1972).
Baan, W. A., and Treves, A., Astr. Astrophys., 22, 421–424 (1973).
Davidson, K., and Ostriker, J. P., Astrophys. J., 179, 585–598 (1973).
Lamb, F. K., Pethick, C. J., and Pines, D., Astrophys. J., 184, 271–289 (1973).
Wang, Y.-M., Astrophys. J. (in the press).
Holt, S. S., Boldt, E. A., Rothschild, R. E., Saba, J. L. R., and Serlemitsos, P. J., Astrophys. J. Lett., 190, L109–L111 (1974).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
WANG, YM. Nature of Her X-1. Nature 253, 249–250 (1975). https://doi.org/10.1038/253249a0
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1038/253249a0
This article is cited by
-
Binary X-ray pulsars
Nature (1977)
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.