Remarks on triaxiality, spin-up, and magnetic field obliquity of some millisecond pulsars

Details Remarks on triaxiality, spin-up, and magnetic field obliquity of some millisecond pulsars Remarks on triaxiality, spin-up, and magnetic field obliquity of some millisecond pulsars

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...390..486c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 390, no. 2, May 10, 1992, p. 486-488. Research supported by University of H

Astronomy and Astrophysics

Astrophysics

3

Globular Clusters, Gravitational Collapse, Neutron Stars, Pulsars, Stellar Rotation, Dipole Moments, Ellipsoids, Magnetic Moments

Scientific paper

The paper shows how two 'observed' properties of millisecond pulsars can find a very natural explanation within the context of the collapse formation and evolution of such objects modeled by uniform density ellipsoids. This model places millisecond pulsars in the neighborhood of the classical bifurcation point between the axisymmetric Maclaurin sequence and the triaxial Jacobi sequence. It is shown that a number of equations of state permit pulsar models to attain a nonaxisymmetric configuration.

Affiliated with

Also associated with

No associations

Rating

Remarks on triaxiality, spin-up, and magnetic field obliquity of some millisecond pulsars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Remarks on triaxiality, spin-up, and magnetic field obliquity of some millisecond pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Remarks on triaxiality, spin-up, and magnetic field obliquity of some millisecond pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1514508