ROSAT observations of V471 Tauri, showing that stellar activity is determined by rotation, not age

Monthly Notices of the Royal Astronomical Society

Volumn 297, Issue 4, 1998, Pages 1145-1150

  Wheatley, Peter J ^a  

^a UNIVERSITY OF LEICESTER   (United Kingdom)

Author keywords

Binaries: close; Novae, cataclysmic variables; Stars: activity; Stars: individual: V471 Tau; White dwarfs; X rays: stars

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; MAGNETIC FIELDS; WHITE DWARFS;

BINARIES: CLOSE; HARD X RAY; NOVAE CATACLYSMIC VARIABLES; SPECTRA'S; STAR: ACTIVITY; STAR: INDIVIDUAL: V471 TAU; STARS: BE; STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAY EMISSION; X-RAY:STARS;

X RAY SCATTERING;

EID: 0040347363     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01607.x     Document Type: Article

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