NGC 7789: AN OPEN CLUSTER CASE STUDY
Autor: | Catherine A. Pilachowski, J. C. Overbeek, Heather R. Jacobson, Szabolcs Mészáros, Christian Johnson, Eileen D. Friel |
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Rok vydání: | 2014 |
Předmět: |
Physics
Metallicity Analytical chemistry FOS: Physical sciences chemistry.chemical_element Astronomy and Astrophysics Barium Astrophysics Spectral line Astrophysics - Solar and Stellar Astrophysics chemistry Space and Planetary Science Arcturus Cluster (physics) Solar and Stellar Astrophysics (astro-ph.SR) Open cluster |
Zdroj: | The Astronomical Journal. 149:15 |
ISSN: | 1538-3881 0004-6256 |
DOI: | 10.1088/0004-6256/149/1/15 |
Popis: | We have obtained high-resolution spectra of 32 giants in the open cluster NGC 7789 using the Wisconsin-Indiana-Yale-NOAO Hydra spectrograph. We explore differences in atmospheric parameters and elemental abundances caused by the use of the linelist developed for the Gaia-ESO Survey (GES) compared to one based on Arcturus used in our previous work. [Fe/H] values decrease when using the GES linelist instead of the Arcturus-based linelist; these differences are probably driven by systematically lower (~ -0.1 dex) GES surface gravities. Using the GES linelist we determine abundances for 10 elements - Fe, Mg, Si, Ca, Ti, Na, Ni, Zr, Ba, and La. We find the cluster's average metallicity [Fe/H] = 0.03 +/- 0.07 dex, in good agreement with literature values, and a lower [Mg/Fe] abundance than has been reported before for this cluster (0.11 +/- 0.05 dex). We also find the neutron-capture element barium to be highly enhanced - [Ba/Fe] = +0.48 +/- 0.08 - and disparate from cluster measurements of neutron-capture elements La and Zr (-0.08 +/- 0.05 and 0.08 +/- 0.08, respectively). This is in accordance with recent discoveries of supersolar Ba enhancement in young clusters along with more modest enhancement of other neutron-capture elements formed in similar environments. 15 pages, 9 figures, Table 1 typo fixed |
Databáze: | OpenAIRE |
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