dc.creatorHorvath, Jorge Ernesto
dc.creatorBenvenuto, Omar Gustavo
dc.date1991-08-15
dc.date2022-10-11T17:18:51Z
dc.date.accessioned2023-07-15T05:12:44Z
dc.date.available2023-07-15T05:12:44Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/143569
dc.identifierissn:0035-8711
dc.identifierissn:1365-2966
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7472505
dc.descriptionStructural constraints are presented on the Crab and Vela pulsars imposed by the simultaneous assumptions of (a) surface temperatures close to those observed by the Einstein Observatory satellite, and (b) 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
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.format670-672
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectEinstein observations
dc.subjectNon-linear regimes
dc.titleEinstein observations and the internal dynamics of compact stars: further evidence against non-linear regimes of vortex creep
dc.typeArticulo
dc.typeArticulo


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