Heavy elements abundances in turn-off stars and early subgiants in NGC 6752

Astronomy and Astrophysics

Volumn 414, Issue 3, 2004, Pages 1071-1079

  James, G ^a   Francois P ^a   Bonifacio, P ^b   Bragaglia, A ^c   Carretta, E ^d   Centurion M ^b   Clementini, G ^c   Desidera, S ^e,f   Gratton, R G ^d   Grundahl, F ^g   Lucatello, S ^d,f   Molaro, P ^b   Pasquini, L ^h   Sneden, C ⁱ   Spite, F ^a  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^c INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^d INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^e UNIVERSITY OF PISA   (Italy)

^f UNIVERSITY OF PADOVA   (Italy)

^g AARHUS UNIVERSITY   (Denmark)

^h EUROPEAN SOUTHERN OBSERVATORY   (Germany)

ⁱ University of Texas at Austin   (United States)

Author keywords

Galaxy: globular clusters: individual: NGC 6752; Stars: abundances

Indexed keywords

GALAXIES; OBSERVABILITY; OBSERVATORIES; SPECTROSCOPY; SPECTRUM ANALYSIS;

GLOBULAR CLUSTER; HALO STARS; HEAVY ELEMENTS; STARS;

ASTRONOMY;

EID: 10744225518     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034014     Document Type: Article

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