X-ray emission from nearby M-dwarfs: The super-saturation phenomenon

Monthly Notices of the Royal Astronomical Society

Volumn 318, Issue 4, 2000, Pages 1217-1226

  James, David J ^a,b   Jardine, Moira M ^a   Jeffries, Robin D ^c   Randich, Sofia ^d   Cameron, Andrew Collier ^a   Ferreira, Miguel ^a  

^a UNIVERSITY OF ST ANDREWS   (United Kingdom)

^b UNIVERSITÉ DE GENÈVE   (Switzerland)

^c KEELE UNIVERSITY   (United Kingdom)

^d INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

Stars: activity; Stars: late type; Stars: rotation; X rays: stars

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; LUMINANCE; ROTATION; STARS;

ACTIVITY LEVELS; ROTATION RATE; SATURATION PHENOMENONS; STAR: ACTIVITY; STARS: ROTATION; STARS:LATE TYPE; SUPER-SATURATION; X-RAY EMISSION; X-RAY LUMINOSITY; X-RAY:STARS;

X RAY SCATTERING;

EID: 0001676779     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03838.x     Document Type: Article

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