Constraining the relative inclinations of the planets B and C of the millisecond pulsar PSR B1257+12

Abstract

We investigate on the relative inclination of the planets B and C orbiting the pulsar PSR B1257+12 in connection with potential violations of the equivalence principle (Abridged).

LaTex2e, 10 pages, 1 table, 3 figures, 17 references. Small stylistic changes. Version to appear in Journal of Astrophysics and Astronomy (JAA)

References in corpus (6)

• The Physics of Neutron Stars
• Precision timing of PSR J0437-4715: an accurate pulsar distance, a high pulsar mass and a limit on the variation of Newton's gravitational constant
• Eight New Millisecond Pulsars in NGC 6440 and NGC 6441
• Masses and orbital inclinations of planets in the PSR B1257+12 system
• A Massive Neutron Star in the Globular Cluster M5
• On the Possibility of Measuring the Gravitomagnetic Clock Effect in an Earth Space-Based Experiment

Cited by in corpus (1)

• Phenomenological constraints on accretion of non-annihilating dark matter on the PSR B1257+12 pulsar from orbital dynamics of its planets