Abundances of microlensed stars in the Bulge Virtual Observatory Resource

Authors

1. Bensby
2. T.
3. Aden
4. D.
5. Melendez
6. J.
7. Gould
8. A.
9. Feltzing
10. S.,Asplund
11. M.
12. Johnson
13. J.A.
14. Lucatello
15. S.
16. Yee
17. J.C.
18. Ramirez
19. I.,Cohen
20. J.G.
21. Thompson
22. I.
23. Gal-Yam
24. A.
25. Han C.
26. Sumi
27. T.
28. Suzuki D.,Wada K.
29. Miyake N.
30. Furusawa K.
31. Ohmori K.
32. Saito To.
33. Tristram P.,Bennett D.

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

2011A&A...533A.134B

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https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/533/A134

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/533/A134

Document Object Identifer DOI

doi:10.26093/cds/vizier.35330134

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