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X-ray emission from A-type stars
Being fully radiative, stars of spectral type A are not expected to harbor magnetic dynamos and hence such stars are not expected to produce X-ray emission.
J. H. M. M. Schmitt, C. Schröder
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X-ray emission from Be star/X-ray binaries
Space Science Reviews, 1994Observations of X-ray emission from Be star/X-ray binaries are reviewed. Some optical characteristics of these binaries are also presented. Theoretical aspects pertaining to the X-ray emissions are given.
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The Sun as an X-Ray Star: Overview of the Method
Solar Physics, 1997We present a method to study the solar-stellar connection, i.e., the close similarity of the physical phenomena occurring on the Sun and on late-type active stars, by taking advantage of Yohkoh/SXT X-ray images. From such images, we first find the distributions of the whole disk differential emission measure, and from them we then synthesize spectra ...
G. PERES +4 more
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Cooling of neutron stars and X-ray observations
Space Science Reviews, 1981Cooling of neutron stars is calculated using an exact stellar evolution code. The full general relativistic version of the stellar structure equations are solved, with the best physical input currently available. For neutron stars with a stiff equation of state, we find that the deviation from the isothermality in the interior is significant and that ...
Ken’ichi Nomoto, Sachiko Tsuruta
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Supersoft X-ray Stars and Supernovae
Scientific American, 1999Kahabka, P. +2 more
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Axion Emission Can Explain a New Hard X-Ray Excess from Nearby Isolated Neutron Stars
Physical Review Letters, 2021Benjamin R Safdi +2 more
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Axion spectra and the associated x-ray spectra of low-mass stars
Physical Review D, 2021Ilidio Lopes
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X-Ray Emission From Utracool Stars
Izvestiya vysshikh uchebnykh zavedenii. Radiofizika, 2021V.V. Zaitsev, A.V. Stepanov
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