Hostname: page-component-848d4c4894-jbqgn Total loading time: 0 Render date: 2024-06-14T07:55:16.917Z Has data issue: false hasContentIssue false
  • English
  • Français

Results of a Search for Visible Pulsars

Published online by Cambridge University Press:  07 February 2017

P. Horowitz ,
C. Papaliolios  and
N. P. Carleton
P. Horowitz
Affiliation:
Harvard University
C. Papaliolios
Affiliation:
Smithsonian Astrophysical Observatory and Harvard University
N. P. Carleton
Affiliation:
Smithsonian Astrophysical Observatory and Harvard University

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 number of interesting celestial objects, including X-ray sources, nova and supernova remnants, white dwarfs, infrared stars, planetary nebulae, radio sources, and some other peculiar nebulosities have been searched with Fourier and correlation techniques for the presence of optical pulsars. The sensitivity of these methods was established with synthetic data and by observations of the Crab Nebula pulsar, the minimum detectable signal (5 standard deviations above noise) being approximately 20th visual magnitude, time averaged. To this limit no new pulsars were found over the range of periods searched from 5 msec to several seconds.

Type
Session 3
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 229 - 233
Copyright
Copyright © Reidel 1971 

References

Horowitz, P.: 1970, ‘Optical Studies of Pulsars’, , .Google Scholar
Kristian, J. and Visvanathan, N., Westphal, J. A., and Snellen, G. H.: 1970, Astrophys. J. 162, 475.CrossRefGoogle Scholar
Lawrence, G. M., Ostriker, J. P., and Hesser, J. E.: 1967, Astrophys. J. 148, L162.CrossRefGoogle Scholar
Neugebauer, G., Martz, D. E., and Leighton, R. B.: 1965, Astrophys. J. 142, 399.Google Scholar
Prentice, A. J. R.: 1970, Nature 225, 438.CrossRefGoogle Scholar
Tucker, W.: 1969, Nature 223, 1250.Google Scholar