Rotational properties of strange stars

Details Rotational properties of strange stars Rotational properties of strange stars

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991nuphs..24..166m&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 24, Issue 2, p. 166-169.

Physics

Nuclear Physics

Scientific paper

Results are presented from studies of the rotational properties of
strange stars concerning, in particular, (i) the changes of mass and
mean radius resulting from rotation; (ii) the minimum rotation period
consistent with stability to non-axisymmetric perturbations.

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