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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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Supersoft X-ray Stars and Supernovae
Scientific American, 1999Kahabka, P. +2 more
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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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Axion Emission Can Explain a New Hard X-Ray Excess from Nearby Isolated Neutron Stars
Physical Review Letters, 2021Malte Buschmann +2 more
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X-ray properties of early-type stars in the Tarantula Nebula from T-ReX
Monthly Notices of the Royal Astronomical Society, 2022Paul A Crowther +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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