An upper limit to optical pulses from the binary pulsar, PSR 1913+16

Details An upper limit to optical pulses from the binary pulsar, PSR 1913+16 An upper limit to optical pulses from the binary pulsar, PSR 1913+16

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...211l.125n&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 211, Feb. 1, 1977, p. L125-L127.

Astronomy and Astrophysics

Astrophysics

9

Binary Stars, Crab Nebula, Optical Properties, Pulsars, Light Curve, Stellar Magnitude, Stellar Spectrophotometry

Scientific paper

An upper limit of magnitude 26.2 is measured for optical pulsations from
PSR 1913+16. If optical pulses from pulsars scale as the inverse n-th
power of period, then by comparison to the Crab pulsar, the limiting
magnitude for PSR 1913+16 requires n to be greater than 9.6.

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