Работы, цитирующие эту работу

Работ: 4

Работа: QPOs during magnetar flares are not driven by mechanical normal modes of the crust

1. Electromagnetic fields in the exterior of an oscillating relativistic star – II. Electromagnetic damping

   Luciano Rezzolla, Bobomurat Ahmedov

   СтатьяPulsars and Gravitational Waves ResearchMonthly Notices of the Royal Astronomical Society2016Цитирований: 11

   ABIABI:AkademIndex/openalex/2026.other.179145

2. Crustal oscillations of slowly rotating relativistic stars

   M. Vavoulidis, Kostas D. Kokkotas, A. Stavridis

   СтатьяPulsars and Gravitational Waves ResearchMonthly Notices of the Royal Astronomical Society2008Цитирований: 2

   ABIABI:AkademIndex/openalex/2008.article.000020

3. Constraints on the magnetic field geometry of magnetars

   H. Sotani, A. Colaiuda, K. D. Kokkotas

   СтатьяPulsars and Gravitational Waves ResearchMonthly Notices of the Royal Astronomical Society2008Цитирований: 1

   ABIABI:AkademIndex/openalex/2026.other.040333

4. Coupled polar-axial magnetar oscillations

   A. Colaiuda, Kostas D. Kokkotas

   СтатьяPulsars and Gravitational Waves ResearchMonthly Notices of the Royal Astronomical Society2012Цитирований: 0

   ABIABI:AkademIndex/openalex/2012.article.000007