The Double Pulsar J0737-3039

Details The Double Pulsar J0737-3039 The Double Pulsar J0737-3039

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ragt.meet..363m&link_type=abstract

In Proceedings of RAGtime 6/7: Workshops on black holes and neutron stars, Opava, 16-18/18-20 September, 2004/2005; S. Hledík an

Astronomy and Astrophysics

Astrophysics

Scientific paper

The discovery of the double pulsar J0737-3039 (Burgay et al., 2003; Lyne et al., 2004) has been a very exciting event for relativistic astrophysics since measurements connected with it are giving the best direct tests so far of the validity of general relativity (see Kramer et al., 2005) and are also allowing new constraints to be placed on the equation of state of neutron star matter (see Podsiadlowski et al., 2005 and references therein). In this paper, we discuss the background to this and describe the results obtained.

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