| Full text | |
| Author(s): Show less - |
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
Total Authors: 14
|
| Document type: | Journal article |
| Source: | PROCEEDINGS OF THE 7TH INTERNATIONAL WORKSHOP ON ASTRONOMY AND RELATIVISTIC ASTROPHYSICS (IWARA 2016); v. 45, p. 7-pg., 2017-01-01. |
| Abstract | |
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) | |
| FAPESP's process: | 13/15088-0 - Magnetars and the highly magnetized, fast, very massive, strange white dwarfs pulsars, and the generation of gravitational waves |
| Grantee: | Jaziel Goulart Coelho |
| Support Opportunities: | Scholarships in Brazil - Post-Doctoral |