Elemental abundances in the center of the Galactic Nuclear Disc
Autor: | Kovtyukh, V. V., Andrievsky, S. M., Martin, R. P., Korotin, S. A., Lepine, J. R. D., Maciel, W. J., , L. E Keir, Panko, E. A. |
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Rok vydání: | 2019 |
Předmět: | |
Druh dokumentu: | Working Paper |
Popis: | We have made the first attempt to derive the chemical properties of the Galactic disc at its very central part using high-resolution infrared spectroscopic observations of four classical Cepheids. Those stars are located at Galactocentric distances smaller than 1 kpc. All investigated stars show near-to-solar elemental abundances. By combining these new data with our previous studies, this result suggests that the radial distribution of iron abundance on a logarithmic scale gradually increases from the outskirts of the Galactic disc to Galactocentric distances of about 2-4 kpc, reaching there a maximal value of about +0.4 dex, and then declines sharply to about the solar value at the Galactic Center. Comment: 7 pages, 5 figures, accepted for publication in MNRAS |
Databáze: | arXiv |
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