Minimal rotation period of strange stars

Details Minimal rotation period of strange stars Minimal rotation period of strange stars

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..954k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, Oct. 1990, p. 954-960. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

5

Peculiar Stars, Stellar Mass, Stellar Rotation, Vacuum Effects, Periodic Variations, Quark Models, Stellar Motions

Scientific paper

Previous estimates of the minimal rotation period of strange stars have
assumed the universality of the bag constant B. For nonuniversal B the
admissible rotation periods are found to be greater than (0.56-0.68) ms.
Hence pulsars with periods smaller than this evidently cannot be
considered as strange stars.

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