Other
Scientific paper
Nov 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988natur.336..226m&link_type=abstract
Nature (ISSN 0028-0836), vol. 336, Nov. 17, 1988, p. 226, 227.
Other
43
Binary Stars, Globular Clusters, Orbital Mechanics, Pulsars, Gravitational Effects, Periodic Variations, Stellar Evolution
Scientific paper
The authors report the results of timing observations of PSR 1620-26, including a first determination of its period derivative P= 3.2±0.4×10-19s s-1 and its orbital eccentricity e = 0.025316±0.000003. The age of this millisecond pulsar is less than 2.2×108years. The relatively high eccentricity is probably a result of gravitational encounters with other stars in the cluster during this time.
Lyne Andrew G.
McKenna Janis
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