Chemical abundances of 11 bulge stars from high-resolution, near-IR spectra

Astronomy and Astrophysics

Volumn 509, Issue 1, 2010, Pages

  Ryde, N ^a,b   Gustafsson, B ^b   Edvardsson, B ^b   Melendez J ^c   Alves Brito, A ^d   Asplund, M ^e   Barbuy, B ^d   Hill, V ^f   Kaufl H U ^g   Minniti, D ^h,i   Ortolani, S ^j   Renzini, A ^k   Zoccali, M ^h  

^a LUND UNIVERSITY   (Sweden)

^b UPPSALA UNIVERSITY   (Sweden)

^c CENTRO DE ASTROFÍSICA   (Portugal)

^d UNIVERSITY OF SÃO PAULO   (Brazil)

^e MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^f UNIVERSITÉ CÔTE D'AZUR   (France)

^g EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^h PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

ⁱ VATICAN OBSERVATORY   (Italy)

^j UNIVERSITY OF PADOVA   (Italy)

^k INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

more..

Author keywords

Abundances Stars; Bulge Infrared; Carbon Galaxy; Late type; Stars; Stars Stars

Indexed keywords

COSMOLOGY; GALAXIES; INFRARED SPECTROSCOPY; OPTICAL TELESCOPES; OXYGEN;

ABUNDANCE RATIOS; ABUNDANCES - STARS; BULGE - INFRARED; CHEMICAL ABUNDANCE; EVOLUTIONARY STAGE; HIGH RESOLUTION; INITIAL MASS; LATE-TYPE STARS; LINE-OF-SIGHT; METALLICITIES; MILKY WAYS; MOLECULAR LINES; NEAR INFRARED SPECTRA; NEAR-IR; OPTICAL SPECTRA; STAR FORMATIONS; STELLAR PARAMETERS; STELLAR POPULATIONS; THICK DISK; VERY LARGE TELESCOPE; WAVELENGTH RANGES;

STARS;

EID: 76349094272     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912687     Document Type: Article

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