Doppler imaging of BD+22°4409 (LO Peg) using least-squares deconvolution

Monthly Notices of the Royal Astronomical Society

Volumn 307, Issue 3, 1999, Pages 685-694

  Lister, T A ^a   Collier Cameron, A ^a   Bartus, J ^b  

^a UNIVERSITY OF ST ANDREWS   (United Kingdom)

^b INSTITUTE OF EXPERIMENTAL MEDICINE   (Hungary)

Author keywords

Line: profiles; Stars: activity; Stars: atmospheres; Stars: individual: BD+22 4409; Stars: late type; Techniques: image processing

Indexed keywords

IMAGE RECONSTRUCTION; LEAST SQUARES APPROXIMATIONS; REPAIR; SIGNAL TO NOISE RATIO; STARS;

CROSS-CORRELATIONS; DECONVOLUTIONS; DOPPLER IMAGING; LINE: PROFILES; STAR: ACTIVITY; STAR: INDIVIDUAL: BD+22°4409; STARS: ATMOSPHERE; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:LATE TYPE; TECHNIQUES: IMAGE PROCESSING;

DOPPLER EFFECT;

EID: 0011034715     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02662.x     Document Type: Article

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