Period variations and phase residuals in freely precessing stars

Details Period variations and phase residuals in freely precessing stars Period variations and phase residuals in freely precessing stars

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...267l..43b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 267, no. 2, p. L43-L46.

Astronomy and Astrophysics

Astrophysics

9

Neutron Stars, Orbital Mechanics, Precession, Variable Stars, Mathematical Models, Stellar Orbits

Scientific paper

An analytical solution is derived for the observed period and phase
variations for a star radiating like a pulsar, which is also freely
precessing like an axisymmetrical rigid body. The disagreements which
arose between Kohabka (1987) and Bisnovatyi-Kogan et al. (1987)
concerning this problem are clarified.

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