Abundances of microlensed Bulge dwarf stars. VI. Virtual Observatory Resource

Authors

1. Bensby T.
2. Feltzing S.
3. Gould A.
4. Yee
5. J.C.
6. Johnson J.A.
7. Asplund M.,Melendez J.
8. Lucatello S.
9. Howes L.M.
10. McWilliam A.
11. Udalski A.,Szymanski M.K.
12. Soszynski I.
13. Poleski R.
14. Wyrzykowski L.
15. Ulaczyk K.,Kozlowski S.
16. Pietrukowicz P.
17. Skowron J.
18. Mroz P.
19. Pawlak
20. M.
21. Abe F.,Asakura Y.
22. Bhattacharya A.
23. Bond I.A.
24. Bennett D.P.
25. Hirao Y.,Nagakane M.
26. Koshimoto N.
27. Sumi T.
28. Suzuki D.
29. Tristram P.J.

Published by

CDS

Abstract

We perform a detailed elemental abundance analysis of dwarf stars in the Galactic bulge, based on high-resolution spectra that were obtained while the stars were optically magnified during gravitational microlensing events. The analysis method is the same as for a large sample of F and G dwarf stars in the Solar neighbourhood, enabling a fully differential comparison between the Bulge and the local stellar populations in the Galactic disc.

Keywords

1. gravitational-lensing
2. chemical-abundances
3. line-intensities

Bibliographic source Bibcode

2017A&A...605A..89B

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ivo://CDS.VizieR/J/A+A/605/A89

Document Object Identifer DOI

doi:10.26093/cds/vizier.36050089

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