Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.

Site Tools

  • AAAS
  • Subscribe
  • Feedback

Site Search

Search Advanced

Science 14 August 1992:
Vol. 257. no. 5072, pp. 937 - 942
DOI: 10.1126/science.257.5072.937

Articles

High-Velocity Pulsars in the Galactic Halo

David Eichler 1 and Joseph Silk 2

1 Department of Physics, Ben Gurion University, Beer Sheva, Israel
2 Departments of Astronomy and Physics and Center for Particle Astrophysics, University of California, Berkeley, CA 94720

It is proposed that high-velocity pulsars are produced in extended galactic halos, and possibly in extragalactic space, from primordial (population III) stars. Such a population of neutron stars could provide an explanation for the gamma-ray bursters and would then accommodate the possibility that most bursters are not in the visible parts of galaxies.

Submitted on February 12, 1992
Accepted on June 23, 1992





ADVERTISEMENT
Click Me!

ADVERTISEMENT
Click Me!

To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)