Standard
A spectroscopy-based age-metallicity relation of the SMC. / Kayser, Andrea; Grebel, E. K.; Harbeck, Daniel et al.
Stellar Populations as Building Blocks of Galaxies. ed. / R. F. Peletier; A. Vazdekis. Vol. 2 Cambridge University Press, 2007. p. 351-352 (Proceedings of the International Astronomical Union; Vol. S241).
Research output: Contribution in Book/Report/Proceedings - With ISBN/ISSN › Conference contribution/Paper › peer-review
Harvard
Kayser, A, Grebel, EK, Harbeck, D, Cole, AA
, Koch, A, Glatt, K, Gallagher III, JS & Da Costa, G 2007,
A spectroscopy-based age-metallicity relation of the SMC. in RF Peletier & A Vazdekis (eds),
Stellar Populations as Building Blocks of Galaxies. vol. 2, Proceedings of the International Astronomical Union, vol. S241, Cambridge University Press, pp. 351-352.
https://doi.org/10.1017/S1743921307008411APA
Kayser, A., Grebel, E. K., Harbeck, D., Cole, A. A.
, Koch, A., Glatt, K., Gallagher III, J. S., & Da Costa, G. (2007).
A spectroscopy-based age-metallicity relation of the SMC. In R. F. Peletier, & A. Vazdekis (Eds.),
Stellar Populations as Building Blocks of Galaxies (Vol. 2, pp. 351-352). (Proceedings of the International Astronomical Union; Vol. S241). Cambridge University Press.
https://doi.org/10.1017/S1743921307008411Vancouver
Kayser A, Grebel EK, Harbeck D, Cole AA
, Koch A, Glatt K et al.
A spectroscopy-based age-metallicity relation of the SMC. In Peletier RF, Vazdekis A, editors, Stellar Populations as Building Blocks of Galaxies. Vol. 2. Cambridge University Press. 2007. p. 351-352. (Proceedings of the International Astronomical Union). doi: 10.1017/S1743921307008411
Author
Kayser, Andrea ; Grebel, E. K. ; Harbeck, Daniel et al. /
A spectroscopy-based age-metallicity relation of the SMC. Stellar Populations as Building Blocks of Galaxies. editor / R. F. Peletier ; A. Vazdekis. Vol. 2 Cambridge University Press, 2007. pp. 351-352 (Proceedings of the International Astronomical Union).
Bibtex
@inproceedings{f4487673f34543b292d23a45e4c44d68,
title = "A spectroscopy-based age-metallicity relation of the SMC",
abstract = "The Small Magellanic Cloud (SMC) is the only dwarf galaxy in the Local Group that is known to have formed and preserved populous star clusters continuously over the past 12 Gyr. Due to its proximity (≈ 60 kpc), stars can be resolved well below the oldest main sequence turnoff points. This facilitates accurate age and metallicity determinations without suffering from the age-metallicity degeneracy. Therefore, the SMC star clusters provide a unique closely spaced set of single-age, single-metallicity tracers to derive a well-sampled age-metallicity relation required for the understanding of the star formation history of this satellite galaxy. Up to date spectroscopically based metallicity estimates exist only for the small number of 7 clusters (Da Costa & Hatzidimitriou 1998). Our project now more than doubles the available data set by the observation of 10 additional clusters.",
author = "Andrea Kayser and Grebel, {E. K.} and Daniel Harbeck and Cole, {Andrew A.} and Andreas Koch and Katharina Glatt and {Gallagher III}, {John S.} and {Da Costa}, G.",
year = "2007",
doi = "10.1017/S1743921307008411",
language = "English",
volume = "2",
series = "Proceedings of the International Astronomical Union",
publisher = "Cambridge University Press",
pages = "351--352",
editor = "Peletier, {R. F.} and A. Vazdekis",
booktitle = "Stellar Populations as Building Blocks of Galaxies",
}
RIS
TY - GEN
T1 - A spectroscopy-based age-metallicity relation of the SMC
AU - Kayser, Andrea
AU - Grebel, E. K.
AU - Harbeck, Daniel
AU - Cole, Andrew A.
AU - Koch, Andreas
AU - Glatt, Katharina
AU - Gallagher III, John S.
AU - Da Costa, G.
PY - 2007
Y1 - 2007
N2 - The Small Magellanic Cloud (SMC) is the only dwarf galaxy in the Local Group that is known to have formed and preserved populous star clusters continuously over the past 12 Gyr. Due to its proximity (≈ 60 kpc), stars can be resolved well below the oldest main sequence turnoff points. This facilitates accurate age and metallicity determinations without suffering from the age-metallicity degeneracy. Therefore, the SMC star clusters provide a unique closely spaced set of single-age, single-metallicity tracers to derive a well-sampled age-metallicity relation required for the understanding of the star formation history of this satellite galaxy. Up to date spectroscopically based metallicity estimates exist only for the small number of 7 clusters (Da Costa & Hatzidimitriou 1998). Our project now more than doubles the available data set by the observation of 10 additional clusters.
AB - The Small Magellanic Cloud (SMC) is the only dwarf galaxy in the Local Group that is known to have formed and preserved populous star clusters continuously over the past 12 Gyr. Due to its proximity (≈ 60 kpc), stars can be resolved well below the oldest main sequence turnoff points. This facilitates accurate age and metallicity determinations without suffering from the age-metallicity degeneracy. Therefore, the SMC star clusters provide a unique closely spaced set of single-age, single-metallicity tracers to derive a well-sampled age-metallicity relation required for the understanding of the star formation history of this satellite galaxy. Up to date spectroscopically based metallicity estimates exist only for the small number of 7 clusters (Da Costa & Hatzidimitriou 1998). Our project now more than doubles the available data set by the observation of 10 additional clusters.
U2 - 10.1017/S1743921307008411
DO - 10.1017/S1743921307008411
M3 - Conference contribution/Paper
VL - 2
T3 - Proceedings of the International Astronomical Union
SP - 351
EP - 352
BT - Stellar Populations as Building Blocks of Galaxies
A2 - Peletier, R. F.
A2 - Vazdekis, A.
PB - Cambridge University Press
ER -
