Recycled radiopulsar reservation in the P-P(dot) diagram

Details Recycled radiopulsar reservation in the P-P(dot) diagram Recycled radiopulsar reservation in the P-P(dot) diagram

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...215l..21k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 215, no. 2, May 1989, p. L21-L23.

Astronomy and Astrophysics

Astrophysics

3

Binary Stars, Pulsars, Radio Stars, Stellar Mass Accretion, Mass Transfer, Stellar Evolution

Scientific paper

The shortest possible period for the pulsar that has undergone accretion in a close binary system is the equilibrium spin period for supercritical accretion rates, of about mu exp 2/3. On the other hand, the period of a pulsar cannot exceed the critical one, P(E), which corresponds to the transition of a magnetized rotator to the propeller state. Those radiopulsars which have originated from binary systems and have passed through an X-ray source stage are situated between the equilibrium period line, P(dot)-P-squared, and the 'suppression line', P(dot)-P-cubed, in the P-P(dot) diagram.

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