| Texto completo | |
| Autor(es): Mostrar menos - |
de Lima, Rafael C. R.
;
Coelho, Jaziel G.
;
Malheiro, Manuel
;
Rueda, Jorge A.
;
Ruffini, Remo
;
DosSantos, AL
;
Vasconcellos, CAZ
;
DaSilva, DT
;
Hadjimichef, D
;
Weber, F
;
Machado, MVT
;
DaSilva, MLL
;
Xu, R
;
Greiner, W
Número total de Autores: 14
|
| Tipo de documento: | Artigo Científico |
| Fonte: | PROCEEDINGS OF THE 7TH INTERNATIONAL WORKSHOP ON ASTRONOMY AND RELATIVISTIC ASTROPHYSICS (IWARA 2016); v. 45, p. 7-pg., 2017-01-01. |
| Resumo | |
We show that nine soft gamma repeaters (SGRs) and Anomalous X-ray Pulsars (AXPs) of the twenty three known sources can be described as rotation-powered canonical pulsars. To accomplish this we use realistic parameters of rotating neutron stars obtained from numerical integration of the self-consistent axisymmetric general relativistic equations of equilibrium. We present limits to the NS mass where the sources can be rotation powered. (AU) | |
| Processo FAPESP: | 13/15088-0 - Magnetares e os pulsares de Anãs Brancas magnetizadas, muito rápidas, massivas e estranhas e a geração de ondas gravitacionais |
| Beneficiário: | Jaziel Goulart Coelho |
| Modalidade de apoio: | Bolsas no Brasil - Pós-Doutorado |