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The Sun as an X-Ray Star: Overview of the Method

Solar Physics, 1997
We 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
openaire   +1 more source

Supersoft X-ray Stars and Supernovae

Scientific American, 1999
Kahabka, P.   +2 more
openaire   +2 more sources

X-Ray Emission From Utracool Stars

Izvestiya vysshikh uchebnykh zavedenii. Radiofizika, 2021
V.V. Zaitsev, A.V. Stepanov
openaire   +1 more source

Axion Emission Can Explain a New Hard X-Ray Excess from Nearby Isolated Neutron Stars

Physical Review Letters, 2021
Malte Buschmann   +2 more
exaly  

X-ray properties of early-type stars in the Tarantula Nebula from T-ReX

Monthly Notices of the Royal Astronomical Society, 2022
Paul A Crowther   +2 more
exaly  

X-Ray Stars

Scientific American, 1967
openaire   +1 more source

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