Possible gravitational amplification in the binary pulsar 1957 + 20

Details Possible gravitational amplification in the binary pulsar 1957 + 20 Possible gravitational amplification in the binary pulsar 1957 + 20

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...214....1s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 214, no. 1-2, April 1989, p. 1-3.

Astronomy and Astrophysics

Astrophysics

5

Companion Stars, Eclipsing Binary Stars, Gravitational Effects, Pulsars, Astronomical Photometry, Brightness, Neutron Stars, Stellar Mass, Stellar Orbits

Scientific paper

For the binary system 1957 + 20, the possible gravitational
amplification of the companion by the pulsar itself is calculated. A
periodic brightness enhancement between 0.0001 and 0.01 is found,
depending on the geometry of the system, with a probability of about 10
percent.

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