On detectability of Zeeman broadening in optical spectra of F- and G-dwarfs

Astronomy and Astrophysics

Volumn 522, Issue 6, 2010, Pages

  Anderson, R I ^a,b   Reiners, A ^b   Solanki, S K ^c,d  

^a UNIVERSITÉ DE GENÈVE   (Switzerland)

^b UNIVERSITY OF GÖTTINGEN   (Germany)

^c MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^d Kyung Hee University   (South Korea)

Author keywords

line: profiles; stars: late type; stars: magnetic field; Sun: surface magnetism; techniques: spectroscopic

Indexed keywords

CONFIDENCE LEVELS; DETECTABILITY; FIT QUALITY; HIGH QUALITY; HOMOGENEOUS DISTRIBUTION; LINE: PROFILES; MAGNETIC REGION; NONMAGNETICS; OPTICAL DATA; OPTICAL SPECTRA; SPECTRAL LINE; STARS: LATE-TYPE; STARS: MAGNETIC FIELD; TC MODEL; TECHNIQUES: SPECTROSCOPIC; TWO-COMPONENT; UPPER LIMITS;

SPECTROSCOPY; STARS;

MAGNETIC FIELDS;

EID: 78149246781     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014769     Document Type: Article

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