Crane, Augmentation, Stellar Astrophysics Binary Pulsar PSR1913+16

Details Crane, Augmentation, Stellar Astrophysics Binary Pulsar PSR1913+16 Crane, Augmentation, Stellar Astrophysics Binary Pulsar PSR1913+16

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.3877c&link_type=abstract

HST Proposal ID #3877

Astronomy and Astrophysics

Astronomy

Hst Proposal Id #3877

Scientific paper

The binary pulsar PSR1913+16, supposedly a prime laboratory for gravitational radiation, may have an optically visible companion, or may be in a visible nebula. WFPC and FOC images will be used to improve the optical astrometry and to study the extension seen in the original images. Since this is such a uniquely important object for our understanding of gravitational radiation, it is crucial to make these definitive observations to clarify the existing uncertainty. If there is an optically luminous companion, or a nebula surrounding the pulsar, this will require modifications to the interpretation of the pulsar timing data.

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