Spectroscopic properties of cool Ursa Major group members

Astronomy and Astrophysics

Volumn 508, Issue 2, 2009, Pages 677-693

  Ammler Von Eiff, M ^a,b,c,d   Guenther, E W ^e  

^a UNIVERSITY OF LISBON   (Portugal)

^b CENTRO DE ASTROFÍSICA   (Portugal)

^c Astophysikalisches Institut   (Germany)

^d UNIVERSITY OF GÖTTINGEN   (Germany)

^e Thüringer Landessterwarte Tautenburg   (Germany)

Author keywords

Open clusters and associations: individual: Ursa Major group solar neighborhood; Stars: abundances; Stars: fundamental parameters

Indexed keywords

DWARF STARS; EFFECTIVE TEMPERATURE; EQUIVALENT WIDTH; GROUP MEMBERS; HIGH RESOLUTION; HIGH SIGNAL-TO-NOISE RATIO; INFILLING; RELATIVE INTENSITY; SOLAR NEIGHBORHOOD; SPECTROSCOPIC PROPERTY; STARS: ABUNDANCES; STARS: FUNDAMENTAL PARAMETERS; STELLAR PARAMETERS;

CHROMOPHORES; COOLING SYSTEMS; IODINE; IRON; KINEMATICS; TEMPERATURE;

STARS;

EID: 77958017704     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912660     Document Type: Article

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