Characteristic times of pulsars and their ages

Details Characteristic times of pulsars and their ages Characteristic times of pulsars and their ages

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986afz....25..525g&link_type=abstract

(Astrofizika, vol. 25, Nov.-Dec. 1986, p. 525-532) Astrophysics (ISSN 0571-7132), vol. 25, no. 3, May 1987, p. 660-664. Translat

Astronomy and Astrophysics

Astrophysics

1

Pulsars, Stellar Evolution, Star Formation, Supernova Remnants

Scientific paper

Three vast regions where the youngest stars located farther than 60 pc, on the average, from the galactic plane are known in the Galaxy. The pulsars with characteristic times τ < 2×106years in these regions deviate in the same direction from the galactic plane as the O-B2 stars. The pulsars with larger values of τ do not show such a correlation. This shows that the pulsars with small τ were formed not long ago and therefore they had no time to leave the region of their birth. For such pulsars τ reflects their age very well.

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