A study of velocity fields in the transition region of ε Eri (K2 V)

Monthly Notices of the Royal Astronomical Society

Volumn 341, Issue 2, 2003, Pages 517-533

  Sim, S A ^a,b   Jordan, C ^a  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b IMPERIAL COLLEGE LONDON   (United Kingdom)

Author keywords

Line: profiles; Stars: chromospheres; Stars: coronae; Stars: individual eridani; Stars: late type

Indexed keywords

ACOUSTIC WAVES; ULTRAVIOLET SPECTROSCOPY; VELOCITY;

ACOUSTICS WAVES; ENERGY FLUXES; LINE: PROFILES; STAR: INDIVIDUAL Ε ERIDANI; STARS: CHROMOSPHERES; STARS: CORONA; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:LATE TYPE; TRANSITION REGIONS; TWO-COMPONENT;

STARS;

EID: 0142105014     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06435.x     Document Type: Review

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