Bayesian timing analysis of giant flare of SGR 180620 by RXTE PCA
V. HambaryanAstrophysikalisches Institut und Universitäts-Sternwarte, Universität Jena, 07745 Jena, GermanyR. NeuhäuserAstrophysikalisches Institut und Universitäts-Sternwarte, Universität Jena, 07745 Jena, GermanyKostas D. KokkotasTheoretical Astrophysics, Eberhard-Karls-Universität Tübingen, 72076 Tübingen, Germany
2011en
ABI
Аннотация
Aims. By detecting high-frequency quasi-periodic oscillations (QPOs) and estimating their frequencies during the decaying tail of giant flares from soft gamma-ray repeaters (SGRs) useful constraints for the equation of state (EoS) of superdense matter may be obtained via comparison with theoretical predictions of eigenfrequencies.
Ҳали таржима қилинмаган
Идентификаторлар
Иқтибослар ва манбалар
2 та иқтибос0 та фойдаланилган манба