HE0056-3022: found in 3 paper(s).

Labels:

/A.E.GarciaPerez et al.(2006)/ /A.E.GarciaPerez et al.(2006)/ /A.Frebel et al.(2006)/

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A0059

Title Li and Be depletion in metal-poor subgiants
ADS A.E.GarciaPerez et al.,AAP, 447, 299, 2006
Authors A. E. Department of Astronomy and Space Physics, UppsalaU. GarciaPerez, F. Primas

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A VLT 55000 100-500 N/A N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Atmospheric data

Teff 5196
log g 2.93+-0.50
vturb 1.5

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Li I...-0.20+-0.092.81+-0.090.96+-0.09
Be II...-3.19+-0.27-0.18+-0.27-2.04+-0.27
Fe...-3.01...4.49
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

A0083

Title Oxygen abundances in metal-poor subgiants as determined from [O I], O I and OH lines
ADS A.E.GarciaPerez et al.,AAP, 451, 621, 2006
Authors A. E. GarciaPerez, M. Asplund, F. Primas, P. E. Nissen, B. Gustafsson

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Basic Informations

Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination -300557.7
Right Ascension 005843.9

Photometric data

V 10.80
V-K 1.973

Atmospheric data

Teff 5196
log g 2.71
vturb 1.5

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
O I...<-2.36<0.65<6.51
OH...-2.490.526.38
Fe II...-3.01+-0.10...4.49+-0.10
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

A0095

Title Bright Metal-poor Stars from the Hamburg/ESO Survey. I. Selection and Follow-up Observations from 329 Fields
ADS A.Frebel et al.,ApJ, 652, 1585, 2006
Authors A. Frebel, N. Christlieb, J. E. Norris, T. C. Beers, M. S. Bessell, J. Rhee, C. Fechner, B. Marsteller, S. Rossi, C. Thom, L. Wisotzki, D. Reimers

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Basic Informations

Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination -300558
Right Ascension 005843.8

Photometric data

B 11.5
B-V 0.69
EB-V 0.02

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
C...-2.410.746.14
Fe...-3.15...4.35
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)