HD97916: found in 6 paper(s).

Labels:

/P.E.Nissen et al.(2002)/ /A.M.Boesgaard(2007)/ /J.P.Fulbright(2000)/ /R.G.Gratton et al.(2003)/ /K.F.Tan et al.(2009)/ /R.Smiljanic et al.(2006)/

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A0048

Title O/Fe in metal-poor main sequence and subgiant stars
ADS P.E.Nissen et al.,AAP, 390, 235, 2002
Authors P. E. Nissen, F. Primas, M. Asplund, D. L. Lambert

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2000-04 N/A VLT 55000 300-400 N/A N/A

Photometric data

V 9.17

Atmospheric data

Teff 6328
log g 4.11
vturb 1.5

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Fe...-0.86...6.64
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


A0125

Title Beryllium in Ultra-Lithium-Deficient Halo Stars:The Blue Straggler Connection
ADS A.M.Boesgaard et al.,ApJ, 667, 1196, 2007
Authors A. M. Boesgaard

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2005-01-31 N/A KECKHIRES N/A 120 20 N/A

Photometric data

V 9.17
B-V 0.38

Atmospheric data

Teff 6375+-81
log g 3.95+-0.20
vturb 1.6

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Li...<0.04<1.00<1.2
Be...<-2.45<-1.49<-1.3
Fe...-0.96+-0.15...6.54+-0.15
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


A0126

Title ABUNDANCES AND KINEMATICS OF FIELD HALO AND DISK STARS. I. OBSERVATIONAL DATA AND ABUNDANCE ANALYSIS
ADS J.P.Fulbright et al.,AJ, 120, 1841, 2000
Authors J. P. Fulbright

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
19990126-31 N/A SANDIFORD N/A 70 3600

Photometric data

V 9.21

Atmospheric data

Teff 6450
log g 4.2
vturb 1.8

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Na I...-0.710.195.62
Mg I...-0.500.47.08
Si I...-0.410.497.14
Ca I...-0.600.35.76
Ti...-0.460.444.56
Cr I...-0.97-0.074.70
Fe...-0.9...6.60
Ba II...-0.850.051.28
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


A0135

Title Abundances for metal-poor stars with accurate parallaxes
ADS R.G.Gratton et al.,AAP, 404, 187, 2003
Authors R. G. Gratton, E. Carretta, R. Claudi, S. Lucatello, M. Barbieri

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A N/A 50000 >100 N/A 55.4
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination 21512
Right Ascension 111554

Binarity

Binarity Positive

Photometric data

V 9.17
B-V 0.42

Atmospheric data

Teff 6412
log g 4.05
vturb 1.26

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Na I...-0.72+-0.0540.19+-0.0545.61+-0.054
Mg I...-0.38+-0.0550.53+-0.0557.20+-0.055
Si I...-0.51+-0.0480.4+-0.0487.04+-0.048
Ca I...-0.58+-0.0330.33+-0.0335.78+-0.033
Ti II...-0.60+-0.0480.31+-0.0484.42+-0.048
Fe I...-0.91+-0.051...6.59+-0.051
Fe II...-0.97+-0.066...6.53+-0.066
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


A0168

Title Beryllium abundances in metal-poor stars
ADS K.F.Tan et al.,MNRAS, 392, 205, 2009
Authors K. F. Tan, J. R. Shi, G. Zhao

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2008-04-10 N/A VLT 48000 N/A N/A N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Atmospheric data

Teff 6350+-80
log g 4.11+-0.15
vturb 1.5+-0.2

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Li...<0.07<0.95<1.23
Be...<-1.91<-1.03<-0.76
O...-0.060.828.81
Ti...-0.650.234.37
Fe...-0.88...6.62
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


A0190

Title Beryllium abundances and star formation in the halo and in the thick disk
ADS R.Smiljanic et al.,ApJ, 644, L121, 2006
Authors R. Smiljanic, L. Pasquini, P. Bonifacio, D. Galli, R. G. Gratton, S. Randich, B. Wolff

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Photometric data

V 9.21

Atmospheric data

Teff 6450
log g 4.05
vturb 1.8

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Li...<0.15<0.95<1.31
Be...<-1.90<-1.10<-0.75
Fe...-0.8...6.70
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)