Cyclotron line signatures of thermal and magnetic mountains from accreting neutron stars
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/445/3/2710/3505465/stu1825.pdf
Reference82 articles.
1. Modelling the spin equilibrium of neutron stars in low-mass X-ray binaries without gravitational radiation
2. Cyclotron Line Features from Near‐critical Magnetic Fields: The Effect of Optical Depth and Plasma Geometry
3. Cyclotron‐Line Features from Near‐Critical Fields. II. On the Effect of Anisotropic Radiation Fields
4. The Limiting Luminosity of Accreting Neutron Stars With Magnetic Fields
5. Spectral formation in accreting X-ray pulsars: bimodal variation of the cyclotron energy with luminosity
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1. Gravitational waves from neutron-star mountains;Classical and Quantum Gravity;2024-01-23
2. Relaxation by thermal conduction of a magnetically confined mountain on an accreting neutron star;Monthly Notices of the Royal Astronomical Society;2018-12-31
3. Revisiting Field Burial by Accretion onto Neutron Stars;Journal of Astrophysics and Astronomy;2017-09
4. Interpreting the AXP 1E 2259+586 antiglitch as a change in internal magnetization;Monthly Notices of the Royal Astronomical Society;2015-08-17
5. Swift/BAT measurements of the cyclotron line energy decay in the accreting neutron star Hercules X-1: indication of an evolution of the magnetic field?;Astronomy & Astrophysics;2015-06
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