activity
19942008
most citedFirst stars VI - Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements

434 citations · 2k across the 23 of their papers we have counts for

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Showing 2006Show all

6 papers · 1 filter

astro-ph2006314 cited

The DART imaging and CaT survey of the Fornax Dwarf Spheroidal Galaxy

G. Battaglia, E. Tolstoy, A. Helmi +13

As part of the DART project we have used the ESO/2.2m Wide Field Imager in conjunction with the VLT/FLAMES GIRAFFE spectrograph to study the detailed properties of the resolved ste…

astro-ph2006115 cited

First stars X. The nature of three unevolved Carbon-Enhanced Metal-Poor stars

T. Sivarani, T. C. Beers, P. Bonifacio +13

From high-resolution VLT/UVES spectra (R~43,000), we determine abundances or upper limits for Li, C, N, O, and other important elements, as well as 12C/13C isotopic ratio for three…

astro-ph2006106 cited

CS 30322-023: an ultra metal-poor TP-AGB star?

T. Masseron, S. Van Eck, B. Famaey +6

With [Fe/H] = -3.5, CS 30322-023 is the most metal-poor star to exhibit a clear s-process signature and the most metal-poor ``lead star'' known. CS 30322-023 is also remarkable in…

astro-ph2006170 cited

First stars IX -Mixing in extremely metal-poor giants. Variation of the 12C/13C, [Na/Mg] and [Al/Mg] ratios

M. Spite, R. Cayrel, V. Hill +11

Extremely metal-poor (EMP) stars preserve a fossil record of the composition of the ISM when the Galaxy formed. It is crucial, however, to verify whether internal mixing has modifi…

astro-ph2006

A VLT-UVES spectrscopic analysis of C-rich Fe-poor stars

T. Masseron, B. Plez, F. Primas +2

Large surveys of very metal-poor stars have revealed in recent years that a large fraction of these objects were carbon-rich, analogous to the more metal-rich CH-stars. The abundan…

astro-ph2006

Element abundances of unevolved stars in the open cluster M 67

S. Randich, P. Sestito, F. Primas +2

We determined the metallicity ([Fe/H]), together with O, Na, Mg, Al, Si, Ca, Ti, Cr and Ni abundances for a sample of 10 unevolved or slightly evolved stars belonging to the open c…