Unpulsed Transient Emission from the PSR B1259--63 System

Details Unpulsed Transient Emission from the PSR B1259--63 System Unpulsed Transient Emission from the PSR B1259--63 System

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atnf.prop.3529j&link_type=abstract

ATNF proposal C326, Semester: October, 2010

Astronomy and Astrophysics

Astronomy

Transients, Atca

Scientific paper

PSR B1259-63 is a pulsar in a highly elliptical, 3.5 year orbit around a Be star companion. Around the time of periastron (the next of which Dec 14, 2010) transient emission is seen at all wavelengths from the radio to the TeV. For this periastron passage we propose a multi-wavelength campaign to understand the origin of the transient emission and to study in detail the shock front between the relativistic pulsar wind and the UV emission from the Be star and disc.

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