Pulsars and Double Pulsars: a Multi-wavelength Approach

Details Pulsars and Double Pulsars: a Multi-wavelength Approach Pulsars and Double Pulsars: a Multi-wavelength Approach

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248...71b&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Astronomy and Astrophysics

Astronomy

2

Radio Sources (Astronomical), X-Ray Sources (Astronomical), Neutron Stars, Nebulae, Solar Electromagnetic Emission, X-Ray Sources, X-Ray Bursts, Neutron Stars, General, Solar Nebula, Cosmogony

Scientific paper

In this paper we will shortly review the multi-wavelength
characteristics of the non-accreting pulsars, focusing on some peculiar
class of objects, and in particular on the high-energy properties of the
first (and unique so-far) double-pulsar system J0737-3039A/B.

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