Detection of a pulsar in a long-period binary system

Details Detection of a pulsar in a long-period binary system Detection of a pulsar in a long-period binary system

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...236l..25m&link_type=abstract

Astrophysical Journal, Part 2-Letters to the Editor, vol. 236, Feb. 15, 1980, p. L25-L27.

Astronomy and Astrophysics

Astrophysics

16

Binary Stars, Pulsars, Cross Correlation, Stellar Models, X Ray Sources

Scientific paper

The paper reports on timing variations, which over a 2 year interval have shown large variations in the period of PSR 0820+02. It is shown that these variations are consistent with the pulsar being a member of a binary system with an orbital period of approximately 1700 days. Finally, it is reported that the corresponding mass function is about 0.023 solar masses.

Affiliated with

Also associated with

No associations

Rating

Detection of a pulsar in a long-period binary system 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 Detection of a pulsar in a long-period binary system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of a pulsar in a long-period binary system will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1620715