output
20022008
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

Showing 2006Show all

12 papers · 1 filter

astro-ph200610 cited

The 2dF BL Lac Survey II

D. Londish, S. M. Croom, J. Heidt +6

We report on our further analysis of the expanded and revised sample of potential BL Lac objects (the 2BL) optically identified from two catalogues of blue-selected (UV excess) poi…

astro-ph200675 cited

Broadband UBVRI Photometry of Horizontal-Branch and Metal-Poor Candidates from the HK and Hamburg/ESO Surveys. I

Timothy C. Beers, Chris Flynn, Silvia Rossi +17

We report broadband UBV and/or BVRI CCD photometry for a total of 1857 stars in the thick-disk and halo populations of the Galaxy. The majority of our targets were selected as cand…

astro-ph200633 cited

A multi-wavelength census of star formation activity in the young embedded cluster around Serpens/G3-G6

A. A. Djupvik, Ph. Andre, S. Bontemps +4

Aims. The aim of this paper is to characterise the star formation activity in the poorly studied embedded cluster Serpens/G3-G6, located ~ 45' (3 pc) to the south of the Serpens Cl…

astro-ph200669 cited

Multifrequency variability of the blazar AO 0235+164. The WEBT campaign in 2004-2005 and long-term SED analysis

C. M. Raiteri, M. Villata, M. Kadler +3

A huge multiwavelength campaign targeting the blazar AO 0235+164 was organized by the Whole Earth Blazar Telescope (WEBT) in 2003-2005 to study the variability properties of the so…

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-ph200613 cited

Short timescale variability in the Faint Sky Variability Survey

L. Morales-Rueda, P. J. Groot, T. Augusteijn +3

We present the V band variability analysis of the point sources in the Faint Sky Variability Survey on time scales from 24 minutes to tens of days. We find that about one percent o…