Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1379...56r&link_type=abstract
ASTROPHYSICS OF NEUTRON STARS 2010: A Conference in Honor of M. Ali Alpar. AIP Conference Proceedings, Volume 1379, pp. 56-59 (
Astronomy and Astrophysics
Astrophysics
Electromagnetic Wave Propagation, Energy Loss Of Particles, Mass, Solar Wind, Electromagnetic Wave Propagation, Energy Loss And Stopping Power, Diameter, Rotation, And Mass, Particle Emission, Solar Wind
Scientific paper
The slow pulsar (J0737-3039B) in the double pulsar system shows drifting features resulting from the emission from the millisecond pulsar in the system (J0737-3039A) interacting with B's magnetosphere. Using a geometrical model [8] that predicts the delay in B's features relative to A's radio pulses, we can constrain some of the properties of this system. We have developed a new methodology to isolate the drifting features from the general B emission. From this, we can determine the sense of rotation of A with respect to its orbit, estimate the altitude of the modulated emission from B due to A, and constrain the angle between the electromagnetic and radio beams.
Freire Paulo C.
McLaughlin Mark Anthony
Rosen Rachel
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