Secular and orbital changes in emission from J0737-3039 system

Details Secular and orbital changes in emission from J0737-3039 system Secular and orbital changes in emission from J0737-3039 system

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..924..591p&link_type=abstract

THE MULTICOLORED LANDSCAPE OF COMPACT OBJECTS AND THEIR EXPLOSIVE ORIGINS. AIP Conference Proceedings, Volume 924, pp. 591-597

Computer Science

Pulsars, Binary And Multiple Stars, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation

Scientific paper

The double-pulsar J0737-3039 is not only the most promising system for testing general relativity, but appears a unique laboratory for investigating the so far unaccessible pulsar magnetosphere and the mechanism for radio emission. In fact, the very high orbital inclination gives the possibility of using the radio beams from pulsar A as a probe for investigating the region close to the surface of pulsar B, while relativistic effects modify the system geometry in a timescale suitable for comparing predictions of various models with observation. We present the status of the multi-wavelength observations performed in the 3 years since the discovery and discuss short and long term perspectives for the study of the magnetosphere of pulsar B.

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