Binary Pulsar PSR1913+16 Imaging

Astronomy and Astrophysics – Astronomy

Scientific paper

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Hst Proposal Id #1061

Scientific paper

A candidate star for the binary pulsar has previously been identified but the precision of the astrometric measurement needs to be improved in order to finally put to rest the question of whether or not this object lies at the radio position. A single 10 minute PC image in the R band will provide the initial data to determine if it is worth using the FGS to get results at the 2 milliarcsec level of precision.

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