An upper limit on optical pulsations from PSR 1913+16

Details An upper limit on optical pulsations from PSR 1913+16 An upper limit on optical pulsations from PSR 1913+16

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...199l.167c&link_type=abstract

Astrophysical Journal, vol. 199, Aug. 1, 1975, pt. 2, p. L167, L168. ERDA-sponsored research.

Astronomy and Astrophysics

Astrophysics

1

Binary Stars, Light Emission, Pulsars, Stellar Radiation, Doppler Effect, Error Analysis, Position (Location), Radio Stars

Scientific paper

A region of the sky covering the 2-min by 2-min error box of PSR 1913+16, a radio pulsar in a binary system, was searched for optical pulsations at the known pulsar frequency. None were observed. An upper limit of 18.2 mag is placed on any such pulsations. Within the smaller error box which has recently been suggested for this object, the limit is 19.2 mag.

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