Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...416..182t&link_type=abstract
Astrophysical Journal v.416, p.182
Astronomy and Astrophysics
Astronomy
21
Galaxy: Stellar Content, Stars: Pulsars: Individual Alphanumeric: Psr J0943+22, Stars: Pulsars: Individual Alphanumeric: Psr J1246+22
Scientific paper
Because ordinary pulsars are distributed in the Galaxy like their massive progenitor stars, sensitive searches for them have been concentrated in the Galactic plane. The greater age and scale height of millisecond pulsars, in contrast, suggest that their local population should be fairly isotropic. We have used the Arecibo radio telescope to search for pulsars in 180 square degrees of sky at high Galactic latitude. We have found two new "slow" pulsars, in addition to detecting the one previously known pulsar in our survey region, but no new millisecond pulsars. The implications for millisecond pulsar population modeling are discussed.
Deich William T. S.
Kulkarni Sanjeev R.
Navarro Jesus
Thorsett Stephen. E.
Vasisht Gautam
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