The fastest rotating pulsar: a strange star?

Authors
Citation
Rx. Xu et al., The fastest rotating pulsar: a strange star?, CHIN PHYS L, 18(6), 2001, pp. 837-840
Citations number
20
Categorie Soggetti
Physics
Journal title
CHINESE PHYSICS LETTERS
ISSN journal
0256307X → ACNP
Volume
18
Issue
6
Year of publication
2001
Pages
837 - 840
Database
ISI
SICI code
0256-307X(200106)18:6<837:TFRPAS>2.0.ZU;2-9
Abstract
According to the observational limits on the radius and mass, the fastest r otating pulsar (PSR 1937+21) is probably a strange star, or at least some n eutron star equations of state should be ruled out, if we suggest that a di pole magnetic field is relevant to its radio emission. We presume that the millisecond pulsar is a strange star with much low mass, small radius and w eak magnetic moment.