Doppler Period Variations of High-Velocity Pulsars

Details Doppler Period Variations of High-Velocity Pulsars Doppler Period Variations of High-Velocity Pulsars

Aug 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971ap%26ss..12..415g&link_type=abstract

Astrophysics and Space Science, Volume 12, Issue 2, pp.415-423

Astronomy and Astrophysics

Astrophysics

Scientific paper

The effect of the source motion on the period variation of pulsars is investigated. For some pulsars, a velocity 100 300 km/s can give a Doppler contribution to the second period derivative P which is comparable or larger than the intrinsic variation predicted by theoretical models, whereas larger velocities are required in order to give an appreciable kinematic effect on the first derivative P. The possibility of experimental detection of P and proper motion for known pulsars is discussed.

Affiliated with

Also associated with

No associations

Rating

Doppler Period Variations of High-Velocity 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 Doppler Period Variations of High-Velocity Pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Doppler Period Variations of High-Velocity Pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1411628