HD201889: found in 5 paper(s).

Labels:

/G.Israelian et al.(2001)/ /T.V.Mishenina et al.(2002)/ /T.V.Mishenina et al.(2001)/ /J.P.Fulbright(2000)/ /R.G.Gratton et al.(2003)/

Find this object in SIMBAD

A0067

Title Sulphur Abundance in Very Metal-poor Stars
ADS G.Israelian et al.,ApJ, 557, L43, 2001
Authors G. Israelian, R. Rebolo

Get more information of this paper.

Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2000-08-17 N/A WHTUES 50000 250 1500 N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Photometric data

V 8.04

Atmospheric data

Teff 5615+-100
log g 4.24+-0.2

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
S...-0.37+-0.10.576.96+-0.1
Fe...-0.94...6.56
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

A0070

Title Abundances of Cu and Zn in metal-poor stars: Clues for Galaxy evolution
ADS T.V.Mishenina et al.,AAP, 396, 189, 2002
Authors T. V. Mishenina, V. V. Kovtyukh, C. Soubiran, C. Travaglio, M. Busso

Get more information of this paper.

Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A ELODIE 42000 >100 N/A N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Fe...-0.78...6.72
Cu I...-0.92+-0.12-0.14+-0.123.29+-0.12
Zn I...-0.84+-0.13-0.06+-0.133.76+-0.13
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

A0071

Title Analysis of neutron capture elements in metal-poor stars
ADS T.V.Mishenina et al.,AAP, 370, 951, 2001
Authors T. V. Mishenina, V. V. Kovtyukh

Get more information of this paper.

Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A ELODIE 42000 >100 N/A N/A

Photometric data

V 8.06
B-V 0.58

Atmospheric data

Teff 5600
log g 4.1
vturb 1.2

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Mg I...-0.680.176.90
Si I...-0.530.327.02
Ca I...-0.500.355.86
Fe...-0.85...6.65
Sr I...-0.750.102.22
Ba II...-0.820.031.31
La II...-0.790.060.38
Ce II...-0.760.090.82
Nd II...-0.840.010.66
    : 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

Get more information of this paper.

Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
1998-07-28 N/A LICKHAMILTON N/A 95 1200

Photometric data

V 8.06

Atmospheric data

Teff 5500
log g 3.9
vturb 1.15

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Na I...-0.730.235.60
Mg I...-0.460.57.12
Al I...-0.550.415.92
Si I...-0.500.467.05
Ca I...-0.520.445.84
Ti...-0.650.314.37
V I...-0.830.133.17
Cr I...-0.910.054.76
Fe...-0.96...6.54
Ni I...-0.910.055.34
Y II...-0.97-0.011.27
Zr II...-0.830.131.77
Ba II...-0.910.051.22
    : 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

Get more information of this paper.

Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A N/A N/A N/A N/A -102.5
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination 241005
Right Ascension 211159

Photometric data

V -81.62

Atmospheric data

Teff 5662
log g 4.08
vturb 1.05

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Na I...-0.64+-0.0540.19+-0.0545.69+-0.054
Mg I...-0.30+-0.0550.53+-0.0557.28+-0.055
Si I...-0.49+-0.0480.34+-0.0487.06+-0.048
Ca I...-0.41+-0.0330.42+-0.0335.95+-0.033
Ti I...-0.58+-0.030.25+-0.034.44+-0.03
Ti II...-0.62+-0.0480.21+-0.0484.40+-0.048
Fe I...-0.83+-0.051...6.67+-0.051
Fe II...-0.9+-0.066...6.60+-0.066
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)