Pairs of pulsars (PSR) and the origin of PSR

Details Pairs of pulsars (PSR) and the origin of PSR Pairs of pulsars (PSR) and the origin of PSR

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.128..363f&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 128, no. 2, Dec. 1986, p. 363-368.

Astronomy and Astrophysics

Astrophysics

1

Binary Stars, Pulsars, Stellar Evolution, Mass Transfer, Stellar Mass

Scientific paper

Research on pairs of pulsars or PSRs which were possibly components of disrupted binaries, seems to advance arguments in favor of the point, that most pulsars were formed in binary systems. Twenty-nine new pairs of pulsars are tabulated that were selected by means of some modifications of the original criteria adopted by Vladimirskii (1984). The averaged value of the time interval between the first and the second supernova outburst was computed for Vladimirskii's list of pairs and the new list. The values, 4.90 and 4.80 million years respectively, are slightly higher than the value obtained in an evolutive model by Van den Heuvel (1976). Correlations between rate of change of period and period for the two lists are examined.

Affiliated with

Also associated with

No associations

Rating

Pairs of pulsars (PSR) and the origin of PSR 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 Pairs of pulsars (PSR) and the origin of PSR, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pairs of pulsars (PSR) and the origin of PSR will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1121320