An analytic treatment of magnetically deformed neutron stars
- 15 April 2021
- journal article
- research article
- Published by Wiley in Astronomische Nachrichten
- Vol. 342 (4), 633-647
- https://doi.org/10.1002/asna.202113862
Abstract
No abstract availableKeywords
Funding Information
- Research Institute for Astronomy and Astrophysics of Maragha (1/6275‐16)
This publication has 59 references indexed in Scilit:
- The force-free twisted magnetosphere of a neutron starMonthly Notices of the Royal Astronomical Society, 2016
- ON MAGNETIC EQUILIBRIA IN BAROTROPIC STARSThe Astrophysical Journal, 2015
- Stability of magnetic fields in non-barotropic stars: an analytic treatmentMonthly Notices of the Royal Astronomical Society, 2013
- Axisymmetric magnetic fields in stars: relative strengths of poloidal and toroidal componentsMonthly Notices of the Royal Astronomical Society, 2009
- Toroidal magnetic fields in type II superconducting neutron starsMonthly Notices of the Royal Astronomical Society, 2008
- Stable magnetic fields in stellar interiorsAstronomy & Astrophysics, 2006
- A fossil origin for the magnetic field in A stars and white dwarfsNature, 2004
- Effects of Strong Magnetic Fields on Neutron Star StructureThe Astrophysical Journal, 2001
- LOCV calculation of nuclear matter with phenomenological two-nucleon interaction operatorsJournal of Physics G: Nuclear and Particle Physics, 1997
- Problems of Gravitational Stability in the Presence of a Magnetic Field.The Astrophysical Journal, 1953