Possible determination of isolated pulsar masses with gravitational microlensing

Details Possible determination of isolated pulsar masses with gravitational microlensing Possible determination of isolated pulsar masses with gravitational microlensing

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.278l..46h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 278, Issue 3, pp. L46-L48.

Astronomy and Astrophysics

Astronomy

1

Gravitation, Pulsars: General, Gravitational Lensing

Scientific paper

An extension of the ongoing gravitational microlensing programmes to the known pulsar population is shown to have the potential of determining isolated pulsar masses with a reasonable precision at a rate of >=2 event century^-1 within the existing sample. Amplification of stars below the detection limit may also occur and add to this rate. Positively detected events would be important for stellar evolution and high-density matter fields.

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