Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aexpr...1...59e&link_type=abstract
Astronomy Express (ISSN 0265-5365), vol. 1, Aug. 1984, p. 59, 60.
Astronomy and Astrophysics
Astronomy
1
Main Sequence Stars, Pulsars, Star Clusters, Stellar Motions, White Dwarf Stars, Radial Velocity, Stellar Color, Stellar Luminosity
Scientific paper
A table is presented which lists some of the observed properties of the pulsars PSRO329+54 and 1929+10 in the Hyades supercluster, as determined from a recent compilation of radio interferometry data by Manchester and Taylor (1981). Values are given for Supercluster parallax errors, dispersion measures, mean electron density along the line of sight, and for the trigonometric parallaxes. It is found that the data support the conclusion that PSRO329+54 and 1929+10 are members of the supercluster. The A-type stars in the Supercluster indicate the possibility of two epochs of star-formation near -10 to the 9th and -(5 to 7) x 10 to the 8th years. The characteristic ages p/2 p-dot are: 5.5 x 10 to the 6th for PSRO329+54; and 3.1 x 10 to the 6th years for 1929+10.
No associations
LandOfFree
Pulsars in the Hyades supercluster 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 Pulsars in the Hyades supercluster, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pulsars in the Hyades supercluster will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1673823