Ushbu ishga iqtibos qilgan ishlar

4 ta ish

Ish: 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

   MaqolaOAOchiq kirishPulsars and Gravitational Waves ResearchMonthly Notices of the Royal Astronomical Society201612 iqtibos

   ABIABI:AkademIndex/2026.other.179145

2. Crustal oscillations of slowly rotating relativistic stars

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

   MaqolaOAOchiq kirishPulsars and Gravitational Waves ResearchMonthly Notices of the Royal Astronomical Society20083 iqtibos

   ABIABI:AkademIndex/2008.article.000020

3. Coupled polar-axial magnetar oscillations

   A. Colaiuda, Kostas D. Kokkotas

   MaqolaOAOchiq kirishPulsars and Gravitational Waves ResearchMonthly Notices of the Royal Astronomical Society20121 iqtibos

   ABIABI:AkademIndex/2012.article.000007

4. Constraints on the magnetic field geometry of magnetars

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

   MaqolaOAOchiq kirishPulsars and Gravitational Waves ResearchMonthly Notices of the Royal Astronomical Society20081 iqtibos

   ABIABI:AkademIndex/2026.other.040333