Physics
Scientific paper
Aug 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.251..670h&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 251, Aug. 15, 1991, p. 670-672. Research supported by C
Physics
1
Heao 2, Massive Stars, Neutron Stars, Stellar Interiors, Crab Nebula, Pulsars, Stellar Physics, Vortices
Scientific paper
Structural constraints are presented on the Crab and Vela pulsars, imposed by the simultaneous assumptions of (1) surface temperatures close to those observed by the Einstein Observatory satellite, and (2) validity of the vortex creep theory in the nonlinear regime for interpreting glitch observations and internal features predicted by it. The disagreement between both studies is quantified, thus pointing strongly to the need for linear regimes of creep, as recently suggested, or some alternative picture.
Benvenuto Omar G.
Horvath Jorge Ernesto
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