Torsional oscillations in neutron star crusts

Details Torsional oscillations in neutron star crusts Torsional oscillations in neutron star crusts

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238..740h&link_type=abstract

Astrophysical Journal, Part 1, vol. 238, June 1, 1980, p. 740-742.

Astronomy and Astrophysics

Astrophysics

37

Astrophysics, Neutron Stars, Oscillations, Stellar Models, Torsional Vibration, Pulsars, Stellar Mass

Scientific paper

The periods of torsional oscillation modes of neutron star crusts are calculated for a range of stellar models. For those with masses greater than about 0.6 solar mass (gravitational) the periods fall into two classes. Those associated with fundamental modes have periods of around 20 ms while higher harmonics are of about 2 ms duration. An identification with subpulse and micropulse pulsar emissions is suggested.

Affiliated with

Also associated with

No associations

Rating

Torsional oscillations in neutron star crusts 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 Torsional oscillations in neutron star crusts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Torsional oscillations in neutron star crusts will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1214705