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@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 = "28 nov. 2020"
}


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