@Article{LimaCoeMalRueRuf:2017:SGRoNe,
author = "Lima, Rafael C. R. and Coelho, Jaziel Goulart and Malheiro, Manuel
and Rueda, Jorge A. and Ruffini, Remo",
affiliation = "{Universidade do Estado de Santa Catarina (UESC)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Tecnol{\'o}gico de Aeron{\'a}utica (ITA)} and {Sapienza
Universit di Roma} and {Sapienza Universit di Roma}",
title = "SGRs/AXPs as rotation-powered neutron stars",
journal = "International Journal of Modern Physics: Conference Series",
year = "2017",
volume = "45",
note = "{7th International Workshop on Astronomy and} and {Relativistic
Astrophysics (IWARA 2016)}",
keywords = "Neutron Star, SGR, AXP.",
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 rotationpowered.",
doi = "10.1142/S2010194517600308",
url = "http://dx.doi.org/10.1142/S2010194517600308",
issn = "2010-1945",
language = "en",
targetfile = "lima_sgrs.pdf",
urlaccessdate = "27 abr. 2024"
}