Wobble radiation from pulsars

Details Wobble radiation from pulsars Wobble radiation from pulsars

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cha%26a..13..345b&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 13, Issue 4, p. 345-349.

Astronomy and Astrophysics

Astrophysics

Pulsars-Gravitational Radiation-Self Gravity

Scientific paper

We derive the post-Newtonian multipole `wobble'' radiation formula taking into account self-gravity, internal stress and internal motion by means of the general multipole-moment formula of Epstein and Wagoner. Applying our formula to the Crab and Vela pulsars, we find the power to be 1.8 times that of the quadrupole radiation. The excess comes mainly from the self-gravity of the source. Thus, it is important to include the self-gravity and to use the antipole-moment formula when considering gravitational radiation from astrophysical sources.

Affiliated with

Also associated with

No associations

Rating

Wobble radiation from pulsars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Wobble radiation from pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Wobble radiation from pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1567775