Standard
Chemical evolution in the Carina dwarf spheroidal. /
Koch, Andreas; Grebel, E. K.; Harbeck, Daniel et al.
Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites. ed. / Sofia Randich; Luca Pasquini. Springer, 2005. p. 249-251 (ESO Astrophysics Symposia).
Research output: Contribution in Book/Report/Proceedings - With ISBN/ISSN › Conference contribution/Paper › peer-review
Harvard
Koch, A, Grebel, EK, Harbeck, D, Wilkinson, MI, Kleyna, J, Gilmore, G, Wyse, RFG & Evans, NW 2005,
Chemical evolution in the Carina dwarf spheroidal. in S Randich & L Pasquini (eds),
Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites. ESO Astrophysics Symposia, Springer, pp. 249-251.
https://doi.org/10.1007/978-3-540-34136-9_82
APA
Koch, A., Grebel, E. K., Harbeck, D., Wilkinson, M. I., Kleyna, J., Gilmore, G., Wyse, R. F. G., & Evans, N. W. (2005).
Chemical evolution in the Carina dwarf spheroidal. In S. Randich, & L. Pasquini (Eds.),
Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites (pp. 249-251). (ESO Astrophysics Symposia). Springer.
https://doi.org/10.1007/978-3-540-34136-9_82
Vancouver
Koch A, Grebel EK, Harbeck D, Wilkinson MI, Kleyna J, Gilmore G et al.
Chemical evolution in the Carina dwarf spheroidal. In Randich S, Pasquini L, editors, Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites. Springer. 2005. p. 249-251. (ESO Astrophysics Symposia). doi: 10.1007/978-3-540-34136-9_82
Author
Bibtex
@inproceedings{bb58adaca643430ebd6966ab60ea7ec7,
title = "Chemical evolution in the Carina dwarf spheroidal",
abstract = "We present metallicities for 487 red giants in the Carina dwarf spheroidal (dSph) galaxy that were obtained from FLAMES low-resolution Ca triplet (CaT) spectroscopy. We find a mean [Fe/H] of –1.91 dex with an intrinsic dispersion of 0.25 dex, whereas the full spread in metallicities is at least one dex. The analysis of the radial distribution of metallicities reveals that an excess of metal poor stars resides in a region of larger axis distances. These results can constrain evolutionary models and are discussed in the context of chemical evolution in the Carina dSph.",
author = "Andreas Koch and Grebel, {E. K.} and Daniel Harbeck and Wilkinson, {M. I.} and Jan Kleyna and G. Gilmore and Wyse, {Rosemary F. G.} and Evans, {N. W.}",
year = "2005",
doi = "10.1007/978-3-540-34136-9_82",
language = "English",
isbn = "9783540341352",
series = "ESO Astrophysics Symposia",
publisher = "Springer",
pages = "249--251",
editor = "Sofia Randich and Luca Pasquini",
booktitle = "Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites",
}
RIS
TY - GEN
T1 - Chemical evolution in the Carina dwarf spheroidal
AU - Koch, Andreas
AU - Grebel, E. K.
AU - Harbeck, Daniel
AU - Wilkinson, M. I.
AU - Kleyna, Jan
AU - Gilmore, G.
AU - Wyse, Rosemary F. G.
AU - Evans, N. W.
PY - 2005
Y1 - 2005
N2 - We present metallicities for 487 red giants in the Carina dwarf spheroidal (dSph) galaxy that were obtained from FLAMES low-resolution Ca triplet (CaT) spectroscopy. We find a mean [Fe/H] of –1.91 dex with an intrinsic dispersion of 0.25 dex, whereas the full spread in metallicities is at least one dex. The analysis of the radial distribution of metallicities reveals that an excess of metal poor stars resides in a region of larger axis distances. These results can constrain evolutionary models and are discussed in the context of chemical evolution in the Carina dSph.
AB - We present metallicities for 487 red giants in the Carina dwarf spheroidal (dSph) galaxy that were obtained from FLAMES low-resolution Ca triplet (CaT) spectroscopy. We find a mean [Fe/H] of –1.91 dex with an intrinsic dispersion of 0.25 dex, whereas the full spread in metallicities is at least one dex. The analysis of the radial distribution of metallicities reveals that an excess of metal poor stars resides in a region of larger axis distances. These results can constrain evolutionary models and are discussed in the context of chemical evolution in the Carina dSph.
U2 - 10.1007/978-3-540-34136-9_82
DO - 10.1007/978-3-540-34136-9_82
M3 - Conference contribution/Paper
SN - 9783540341352
T3 - ESO Astrophysics Symposia
SP - 249
EP - 251
BT - Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites
A2 - Randich, Sofia
A2 - Pasquini, Luca
PB - Springer
ER -
