The 6.7 keV thermal emission lines in the stellar flare spectra of two chromospherically active Binaries: Algol and GT Mus-Reference-Cited by-同舟云学术

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The 6.7 keV thermal emission lines in the stellar flare spectra of two chromospherically active Binaries: Algol and GT Mus

Published:2022-01 Issue:1 Volume:69 Page:499-513
ISSN:0273-1177
Container-title:Advances in Space Research
language:en
Short-container-title:Advances in Space Research

Author:

Eze Ambrose Chukwudi,Esaenwi Sudum,Madu Fidelis Okey

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference107 articles.

1. ASCA observations of the coronal X-ray emission of Algol;Antunes;Astrophys J,1994

2. A study of coronal abundances in RS CVn binaries*;Audard;Astronomy&Astrophysics,2003

3. Imaging the Algol Triple system in the H Band with the Chara Interferometer;Baron;Astrophys J,2012

4. The age-mass relation for chromospherically active binaries III. Lithium depletion in giant components*;Barrado;A & A,1998

5. The age-mass relation for chromospherically active binaries II. Lithium depletion in dwarf components***;Barrado;A & A,1997

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