VLBI of the PSR B1259-63 system

Details VLBI of the PSR B1259-63 system VLBI of the PSR B1259-63 system

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atnf.prop..902j&link_type=abstract

ATNF proposal V234, Semester: April, 2007

Astronomy and Astrophysics

Astronomy

Stellar, Galactic, Lba

Scientific paper

PSR B1259-63 is a binary system consisting of a young pulsar and a massive Be star. It shows transient emission near periastron, which next occurs in July 2007. We propose observations to (a) test the predictions made for the location and nature of the transient emission (b) measure the angular size of the orbit and hence a precise distance and (c) measure the proper motion of the system. The new broadband VLBI system makes such an experiment possible.

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