Release 11.12 ("Hergest Ridge")
Article ID: gc523 | |
Author | Lamb, M. P.; Venn, K. A.; Shetrone, M. D.; Sakari, C. M.; Pritzl, B. J. |
Title | Chemical abundances in the globular clusters NGC 5024 and NGC 5466 from optical and infrared spectroscopy |
Journal | MNRAS, Volume 448, Issue 1, p.42-58 |
Year of publication | 2015 (on gclusters from 2017-02-06 10:57:52 ) |
Abstract | Detailed chemical abundances for five stars in two Galactic globular clusters, NGC 5466 and NGC 5024, are presented from high-resolution optical (from the Hobby-Eberley Telescope) and infrared spectra (from the SDSS-III APOGEE survey). We find [Fe/H] = -1.97 ± 0.13 dex for NGC 5466, and [Fe/H] = -2.06 ± 0.13 dex for NGC 5024, and the typical abundance pattern for globular clusters for the remaining elements, e.g. both show evidence for mixing in their light element abundance ratios (C, N), and asymptotic giant branch contributions in their heavy element abundances (Y, Ba, and Eu). These clusters were selected to examine chemical trends that may correlate them with the Sgr dwarf galaxy remnant... |
Also available at: | https://arxiv.org/abs/1412.5210 |
Submitted by | Paolo Ventura |
Tags | NGC 5024 , NGC 5466 |
This page has been visited 923 times since March, 14 2013
Query processed at 20:38, 31st May
Home | | Parameters | | Table 1 | | Table 2 | | Table 3 |
Search | | Feedback | | What's new | | Links | | Blog |