Abstract
WE report a measurement of the pulsed X-ray emission associated with the pulsar NP 0532 in the Crab Nebula. This information was obtained with a six element detector flown on an Aerobee 150 rocket from White Sands N. M., launched on March 16, 1968, at 0315 UT. Our results on the overall 2–20 keV spectrum from the Crab Nebula and the diffuse X-ray background, as well as a payload description, have been published elsewhere1.
Similar content being viewed by others
References
Boldt, E. A., Desai, U. D., and Holt, S. S., Astrophys. J., 156, 427 (1969).
Cocke, W. J., Disney, M. J., and Taylor, D. J., Nature, 221, 525 (1969).
Warner, B., Nather, R. E., and McFarlane, M., Nature, 222, 233 (1969).
Fritz, G., Henry, R. C., Meekins, J. F., Chubb, T. A., and Friedman, H., Science, 164, 709 (1969).
Bradt, H., Rappaport, S., Mayer, W., Nather, R. E., Warner, B., McFarlane, M., and Kristian, J., Nature, 222, 728 (1969).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
BOLDT, E., DESAI, U., HOLT, S. et al. Pulsed X-ray Emission of NP 0532 in March 1968. Nature 223, 280–281 (1969). https://doi.org/10.1038/223280a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/223280a0
- Springer Nature Limited
This article is cited by
-
Pulsars. Survey of observational data
Astrophysics (1980)
-
Transient structure in the high-energy X-ray light curve of NP 0532
Nature (1977)
-
X-ray spectrum of NP0532
Nature (1974)
-
The crab nebula
Astrophysics and Space Science (1973)
-
Measurement of the Pulsation Ratio of the Crab Nebula in the X-ray Region from 20 to 80 keV
Nature Physical Science (1971)