Astronomy and Astrophysics, 480, pp. 379-395, http://dx.doi.org./10.1051/0004-6361:20064854
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2008 (v1)Journal articleUploaded on: December 4, 2022
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June 2021 (v1)Publication
The UltraViolet-Visual Echelle Spectrograph (UVES) was first offered to the ESO community in 2000. A workhorse covering a vast range of topics from Solar System objects to cosmology, it quickly became one of the most productive instruments at Paranal. For the 20th anniversary of UVES's entering into service, over 100 astronomers from across the...
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2012 (v1)Journal article
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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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October 2020 (v1)Journal article
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2011 (v1)Journal article
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2010 (v1)Journal article
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2009 (v1)Journal article
Astronomy and Astrophysics, 501, pp. 519-530 (2009)
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2010 (v1)Journal article
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August 10, 2009 (v1)Conference paper
The abundance derivation of heavy r-elements may provide a better understanding of the r-process, and the determination of several reference r-elements should allow a better determination of the star's age. The spatial ultraviolet (UV) region presents a large number of lines of heavy elements, and in some cases such as Bi, Pt, Au, detectable...
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2011 (v1)Journal article
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2011 (v1)Journal article
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May 19, 2013 (v1)Conference paper
As a brief revision, the origin of heavy elements and the role of abundances in extremely metal-poor (EMP) stars are presented. Heavy element abundances in the EMP uranium-rich star CS 31082-001 based mainly on near-UV spectra from STIS/HST are presented. These results should be useful for a better characterisation of the neutron exposure(s)...
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2011 (v1)Journal article
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2015 (v1)Journal article
We present new homogeneous measurements of Na, Al, and three alpha-elements (Mg, Si, Ca) for 75 Galactic Cepheids. The abundances are based on high spectral resolution (R~ 38 000) and high signal-to-noise ratio (S/N ~ 50-300) spectra collected with UVES at ESO VLT. The current measurements were complemented with Cepheid abundances provided by...
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2012 (v1)Journal article
International audience
Uploaded on: December 3, 2022