Abundances of microlensed stars in the Bulge


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.

Cone search capability for table J/A+A/512/A41/table1 (Summary of the so far 15 dwarf star microlensing events in the Bulge that have been observed with high-resolution spectrographs)

DOI http://doi.org/10.26093/cds/vizier.35120041
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/512/A41
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/512/A41
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/512/A41
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/512/A41
Creator Bensby T.; Feltzing S.; Johnson J.A.; Gould A.; Aden D.; Asplund M.; Melendez J.; Gal-Yam A.; Lucatello S.; Sana H.; Sumi T.; Miyake N.; Suzuki N.; Han C.; Bond I.; Udalski A.
Publisher CDS
Publication Year 2010
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Resource Type Dataset
Discipline Astrophysical Processes; Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Physics