Dependence of pulsewidth on the age of pulsars - A comment on candy and Blair's analysis

Details Dependence of pulsewidth on the age of pulsars - A comment on candy and Blair's analysis Dependence of pulsewidth on the age of pulsars - A comment on candy and Blair's analysis

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.214p..15k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 214, May 1, 1985, p. 15P-17P.

Astronomy and Astrophysics

Astronomy

3

Emission Spectra, Pulsars, Pulse Duration, Stellar Evolution, Axes Of Rotation, Data Processing

Scientific paper

Candy and Blair have found that pulsewidth depends on the characteristic
age of a pulsar and suggest that the emission cone aligns with the spin
axis on a time-scale of ≡107yr. A re-examination of the
data used by them reveals no evidence for the reported dependence.

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