Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...152...89h&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 152, no. 1, Nov. 1985, p. 89-92.
Astronomy and Astrophysics
Astrophysics
2
Pulsars, Statistical Distributions, Stellar Evolution, Chronology, Stellar Magnetic Fields, Stellar Motions
Scientific paper
Based on an earlier proposal that pulsars be separated into two types, the z distribution and characteristic ages of Type II candidates (with periods less than 0.5 s) and Type I pulsars (with periods greater than 1.3 s) are reexamined. It is shown that the characteristic ages for Type II candidates and for pulsars with periods less than 0.5 s can be used as the upper limit of their true ages, which may be less than or equal to 5 x 10 to the 6th years. The true ages of type I pulsars are larger than 10 million years. The scale heights of the two types also vary differently with period and characteristic age.
Huang Jia-Hong
Huang Ke-Liang
Peng Qiu He
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