JINA - Virtual Journal of Nuclear Astrophysics,
27 November 2009
Volume 7, Issue 48 (34 Articles)
- # 4 - Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. II. Ages, metallicities, detailed elemental abundances, and connections to the Galactic thick disc
- T. Bensby (1), S. Feltzing (2), J.A. Johnson (3), A. Gould (3), D. Adén (2), M. Asplund (4), J. Meléndez (5), A. Gal-Yam (6), S. Lucatello, (7) H. Sana (1 and 8), T. Sumi (9), N. Miyake (9), D. Suzuki (9), C. Han (10), I. Bond (11), A. Udalski (12) ((1) ESO, Chile, (2) Lund Observatory, Sweden, (3) Ohio state Univ., USA, (4) MPA-Garching, Germany, (5) Universidade do Porto, Portugal, (6) Benoziyo Center for Astrophysics, Weizmann Inst of Science, Israel, (7) INAF, Padova, Italy, (8) Universiteit van Amsterdam, Sterrenkundig Instituut, Netherlands, (9) Solar-Terrestrial Environment Laboratory, Nagoya Univ., Japan, (10) Chungbuk National Univ, Republic of Korea, (11) Massey Univ., New Zealand, (12) Warzaw University Observatory, Poland)
- arXiv.org - Astrophysics - Volume: 2009, Issue: 26 Nov
- arXiv:0911.5076 [ps, pdf, other]
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.
