Cyclotron harmonics in opacities of isolated neutron star atmospheres
arXiv:1003.5106 · doi:10.1051/0004-6361/201014781
Abstract
Some of X-ray dim isolated neutron stars (XDINS) and central compact objects in supernova remnants (CCO) show absorption features in their thermal soft X-ray spectra. It has been hypothesized that these features could be due to the periodic peaks in free-free absorption opacities, caused by either Landau quantization of electron motion in magnetic fields B<10^{11} G or analogous quantization of ion motion in magnetic fields B>10^{13} G. Here, I review the physics behind cyclotron quantum harmonics in free-free photoabsorption, discuss different approximations for their calculation, and explain why the ion cyclotron harmonics (beyond the fundamental) cannot be observed.
12 pages, 5 figures. In v.5, a typo (missed sign factor) in Eq.(9) is fixed
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- Central Compact Objects in Supernova Remnants
- The Hidden Magnetic Field of The Young Neutron Star in Kesteven 79
- On the compactness of the isolated neutron star RX J0720.4-3125
- Constraining the Neutron Star Mass--Radius Relation and Dense Matter Equation of State with NICER. III. Model Description and Verification of Parameter Estimation Codes
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- Neutron stars - thermal emitters
- Low-magnetic-field magnetars
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- Mean opacities of a strongly magnetized high temperature plasma