Annual Review of Astronomy and Astrophysics, 47, pp. 371-425 (2009)
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2009 (v1)Journal articleUploaded on: December 3, 2022
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October 2017 (v1)Journal article
From ESO VLT/FLAMES/GIRAFFE spectra, abundance measurements of Zn have been made in ≈100 individual red giant branch (RGB) stars in the Sculptor dwarf spheroidal galaxy. This is the largest sample of individual Zn abundance measurements within a stellar system beyond the Milky Way. In the observed metallicity range, -2.7
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July 2018 (v1)Journal article
Abundances of the volatile elements S and Zn have now been measured in around 80 individual stars in the Sculptor dwarf spheroidal galaxy, covering the metallicity range - 2.4 ≤ [Fe/H] ≤-0.9. These two elements are of particular interest as they are not depleted onto dust in gas, and their ratio, [S/Zn], has thus commonly been used as a proxy...
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2008 (v1)Journal article
Astrophysical Journal, 681, pp. L13-L16, http://dx.doi.org./10.1086/590179
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2011 (v1)Journal article
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2008 (v1)Journal article
We demonstrate that low-resolution Ca II triplet (CaT) spectroscopic estimates of the overall metallicity ([Fe/H]) of individual red giant branch (RGB) stars in two nearby dwarf spheroidal galaxies (dSphs) agree to ±0.1-0.2 dex with detailed high-resolution spectroscopic determinations for the same stars over the range −2.5 < [Fe/H] < −0.5. For...
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2012 (v1)Journal article
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2012 (v1)Journal article
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2022 (v1)Journal article
The tidal tails of Palomar 5 (Pal 5) have been the focus of many spectroscopic studies in an attempt to identify individual stars lying along the stream and characterize their kinematics. The well-studied trailing tail has been explored out to a distance of 15○ from the cluster centre, while less than 4° have been examined along the leading...
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December 1, 2020 (v1)Journal article
We present the high-resolution spectroscopic analysis of two new extremely metal-poor stars (EMPS) candidates in the dwarf spheroidal galaxy Sextans. These targets were pre-selected from medium resolution spectra centered around the Ca II triplet in the near-infrared and followed-up at higher resolution with VLT/UVES. We confirm their low...
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2017 (v1)Journal article
We confirm the reality of the recently discovered Milky Way stellar cluster Gaia 1 using spectra acquired with the HERMES and AAOmega spectrographs of the Anglo-Australian Telescope. This cluster had been previously undiscovered due to its close angular proximity to Sirius, the brightest star in the sky at visual wavelengths. Our observations...
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2010 (v1)Journal article
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2009 (v1)Journal article
Astronomy and Astrophysics, 501, pp. 189-206 (2009)
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2011 (v1)Journal article
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June 2019 (v1)Journal article
We present detailed chemical abundances for 99 red-giant branch stars in the centre of the Sculptor dwarf spheroidal galaxy, which have been obtained from high-resolution VLT/FLAMES spectroscopy. The abundances of Li, Na, α-elements (O, Mg, Si, Ca Ti), iron-peak elements (Sc, Cr, Fe, Co, Ni, Zn), and r- and s-process elements (Ba, La, Nd, Eu)...
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2010 (v1)Journal article
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2011 (v1)Journal article
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2011 (v1)Journal article
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2012 (v1)Journal article
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December 2014 (v1)Journal article
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October 2020 (v1)Journal article
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May 2018 (v1)Journal article
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2010 (v1)Journal article
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