Recent observations of BSR B1534+12

Details Recent observations of BSR B1534+12 Recent observations of BSR B1534+12

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001iaus..205..408s&link_type=abstract

Galaxies and their Constituents at the Highest Angular Resolutions, Proceedings of IAU Symposium #205, held 15-18 August 2000 at

Physics

Scientific paper

We present the results of recent Arecibo observations of the relativistic double-neutron-star binary PSR B1534+12. The timing solution includes measurements of five post-Keplerian orbital parameters, whose values agree well with the predictions of general relativity. The observations show that the pulse profile is evolving secularly at both 1400 MHz and 430 MHz. This effect is similar to that seen in PSR B1913+16, and is almost certainly due to general relativistic precession of the pulsar's spin axis. We also present high-quality polarimetric profiles at both observing frequencies.

Affiliated with

Also associated with

No associations

Rating

Recent observations of BSR B1534+12 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 Recent observations of BSR B1534+12, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Recent observations of BSR B1534+12 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1363252