A new look at the relationship between activity, dynamo number and Rossby number in late-type stars

Monthly Notices of the Royal Astronomical Society

Volumn 326, Issue 3, 2001, Pages 877-884

  Montesinos, B ^a,b   Thomas, John H ^c   Ventura, P ^d   Mazzitelli, I ^e  

^a INSTITUTO NACIONAL DE TÉCNICA AEROESPACIAL   (Spain)

^b INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^c University of Rochester   (United States)

^d INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^e CNR   (Italy)

Author keywords

Convection; Stars: activity; Stars: chromospheres; Stars: rotation

Indexed keywords

INTERACTIVE DEVICES; MAGNETIC FIELDS; ROTATION; TURBULENCE;

CONVECTION; DIFFERENTIAL ROTATION; DYNAMO THEORIES; LATE-TYPE STARS; ROSSBY NUMBERS; SOLAR DYNAMO; STAR: ACTIVITY; STARS: BE; STARS: CHROMOSPHERES; STARS: ROTATION;

STARS;

EID: 0001603425     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04476.x     Document Type: Article

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