Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars: IV. Two bulge populations

Astronomy and Astrophysics

Volumn 533, Issue , 2011, Pages

  Bensby, T ^a,b   Aden D ^a   Melendez J ^c   Gould, A ^d   Feltzing, S ^a   Asplund, M ^e   Johnson, J A ^d   Lucatello, S ^f   Yee, J C ^d   Ramirez I ^g   Cohen, J G ^h   Thompson, I ^g   Bond, I A ⁱ   Gal Yam, A ^j   Han, C ^k   Sumi, T ^l   Suzuki, D ^l   Wada, K ^l   Miyake, N ^m   Furusawa, K ^m   Ohmori, K ^m   Saito, To ⁿ   Tristram, P ^o   Bennett, D ^p   more..

^a LUND UNIVERSITY   (Sweden)

^b EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^c UNIVERSITY OF SÃO PAULO   (Brazil)

^d OHIO STATE UNIVERSITY   (United States)

^e MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^f INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^g CARNEGIE OBSERVATORIES   (United States)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ MASSEY UNIVERSITY   (New Zealand)

^j WEIZMANN INSTITUTE OF SCIENCE   (Israel)

^k Chungbuk National University   (South Korea)

^l OSAKA UNIVERSITY   (Japan)

^m NAGOYA UNIVERSITY   (Japan)

ⁿ TOKYO METROPOLITAN COLLEGE OF INDUSTRIAL TECHNOLOGY   (Japan)

^o UNIVERSITY OF AUCKLAND   (New Zealand)

^p UNIVERSITY OF NOTRE DAME   (United States)

more..

Author keywords

Galaxy: bulge; Galaxy: evolution; Galaxy: formation; Gravitational lensing: micro; Stars: abundances

Indexed keywords

GALAXY: BULGE; GALAXY: EVOLUTION; GALAXY: FORMATION; GRAVITATIONAL LENSING; STARS: ABUNDANCES;

ASTROPHYSICS; BARIUM; CHROMIUM; GALAXIES; METALS; SODIUM;

STARS;

EID: 80052855851     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117059     Document Type: Article

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