Dependence of coronal X-ray emission on spot-induced brightness variations in cool main sequence stars

Astronomy and Astrophysics

Volumn 410, Issue 2, 2003, Pages 671-684

  Messina, S ^a   Pizzolato, N ^b   Guinan, E F ^c   Rodono M ^d  

^a INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^c VILLANOVA UNIVERSITY   (United States)

^d UNIVERSITY OF CATANIA   (Italy)

Author keywords

Stars: activity; Stars: late type; Stars: magnetic fields; Stars: starspots; X ray: stars

Indexed keywords

BOLOMETERS; MAGNETIC FIELD EFFECTS; PHOTOMETRY; SOLAR SYSTEM; STATISTICAL METHODS;

COOL MAIN SEQUENCE STARS; CORONAL X RAY EMISSION; PHOTOSPHERIC CORONAL ACTIVITY; SPOT INDUCED BRIGHTNESS VARIATION;

ASTROPHYSICS;

EID: 0242354962     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031203     Document Type: Article

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