%0 Journal Article
%@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}
%@nexthigherunit 8JMKD3MGPCW/3ETR8EH
%2 sid.inpe.br/mtc-m21b/2017/11.03.14.12.40
%4 sid.inpe.br/mtc-m21b/2017/11.03.14.12
%3 lima_sgrs.pdf
%9 conference paper
%@issn 2010-1945
%A Lima, Rafael C. R.,
%A Coelho, Jaziel Goulart,
%A Malheiro, Manuel,
%A Rueda, Jorge A.,
%A Ruffini, Remo,
%@secondarytype PRE PI
%B International Journal of Modern Physics: Conference Series
%D 2017
%K Neutron Star, SGR, AXP.
%@archivingpolicy denypublisher allowfinaldraft
%O 7th International Workshop on Astronomy and
%O Relativistic Astrophysics (IWARA 2016)
%@secondarymark B4_ENGENHARIAS_III C_ASTRONOMIA_/_FÍSICA
%T SGRs/AXPs as rotation-powered neutron stars
%V 45
%X 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 rotationpowered.
%@area CEA
%@electronicmailaddress rafael.camargo@icranet.org
%@electronicmailaddress jaziel.coelho@inpe.br
%@electronicmailaddress malheiro@ita.br
%@electronicmailaddress jorge.rueda@icra.it
%@electronicmailaddress ruffini@icra.it
%@documentstage not transferred
%@group
%@group DIDAS-CGCEA-INPE-MCTIC-GOV-BR
%@dissemination WEBSCI; PORTALCAPES; COMPENDEX.
%@usergroup simone
%@affiliation Universidade do Estado de Santa Catarina (UESC)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Tecnológico de Aeronáutica (ITA)
%@affiliation Sapienza Universit di Roma
%@affiliation Sapienza Universit di Roma
%@versiontype publisher
%@doi 10.1142/S2010194517600308