$\mathsf{\alpha}$-, r -, and s -process element trends in the Galactic thin and thick disks
Netherlands Institute for Radio Astronomy · University of Michigan–Ann Arbor · +2 more institutions
Abstract
From a detailed elemental abundance analysis of 102 F and G dwarf stars we present abundance trends in the Galactic thin and thick disks for 14 elements (O, Na, Mg, Al, Si, Ca, Ti, Cr, Fe, Ni, Zn, Y, Ba, and Eu). Stellar parameters and elemental abundances (except for Y, Ba and Eu) for 66 of the 102 stars were presented in our previous studies (Bensby et al. [CITE], A&A, 410, 527, [CITE], A&A, 415, 155). The 36 stars that are new in this study extend and confirm our previous results and allow us to draw further conclusions regarding abundance trends. The s-process elements Y and Ba, and the r-element Eu have also been considered here for the whole sample for the first time. With this new larger sample we now…
Citation impact
- FWCI
- 22.92
- Percentile
- 100%
- References
- 66
Authors
4- TBT. BensbyCorresponding
Netherlands Institute for Radio Astronomy, University of Michigan–Ann Arbor, Lund University
- SFS. Feltzing
Netherlands Institute for Radio Astronomy, Lund University
- ILIngemar Lundström
Lund University, Netherlands Institute for Radio Astronomy
- III. Ilyin
Leibniz Institute for Astrophysics Potsdam
Topics & keywords
- Stars
- Astrophysics
- Thin disk
- Thick disk
- Physics
- Galaxy
- Disc
- Abundance (ecology)