Rapidly Rotating Neutron Stars

Details Rapidly Rotating Neutron Stars Rapidly Rotating Neutron Stars

May 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973phrvl..30.1082w&link_type=abstract

Physical Review Letters, vol. 30, Issue 21, pp. 1082-1084

Physics

16

Scientific paper

Models of differentially rotating neutron stars have been calculated. An
upper limit to the rotational enhancement of the maximum gravitational
mass is found to be about 50% when the Ostriker-Tassoul instability
criterion is used.

Affiliated with

Also associated with

No associations

Rating

Rapidly Rotating Neutron Stars 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 Rapidly Rotating Neutron Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rapidly Rotating Neutron Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1669701