HD21581
HIP16214 in K.A.Venn+,AJ, 128, 1177, 2004
taken from 10 paper(s):
/R.G.Gratton et al.(2000)/
/J.Melendez and B. Barbuy(2001)/
/J.P.Fulbright and J. A. Johnson(2003)/
/J.P.Fulbright(2000)/
/J.Simmerer et al.(2004)/
/B.W.Carney et al.(2003)/
/Y.Saito et al.(2009)/
/I.U.Roederer et al.(2010)/
/H.Jonsson et al.(2011)/
/I.U.Roederer et al.(2014)/
Mixing along the red giant branch in metal-poor field stars
Stellar Parameters
Teff : 4978 | log g : 2.29 | vturb : 1.30 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li I | N/A | ... | ... | 0.95 | -2.31 | -0.70 | 0.95 | Li I |
C | N/A | ... | -0.25 | ... | -1.74 | -0.13 | 6.69 | C |
CN | N/A | ... | -0.25 | ... | -1.64 | -0.03 | 6.19 | CN |
O | N/A | ... | 0.26 | ... | -1.12 | 0.49 | 7.57 | O |
[O I] | N/A | ... | 0.39 | ... | -0.99 | 0.62 | 7.70 | [O I] |
Na | N/A | ... | -0.11 | ... | -1.68 | -0.07 | 4.56 | Na |
Fe I | N/A | -1.56 | ... | ... | -1.61 | ... | 5.89 | Fe I |
Fe II | N/A | -1.62 | ... | ... | -1.67 | ... | 5.83 | Fe II |
Isotopic Ratio
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1995-05 | N/A | CESESO | 50000 | 80-150 | N/A | N/A |
1995-11 | N/A | CESESO | 50000 | 80-150 | N/A | N/A |
1995-11 | N/A | MCDONALD | 60000 | 70-100 | N/A | N/A |
Oxygen Abundances in Metal-poor Stars (-2.2 < [Fe/H] < -1.2) from Infrared OH Lines
Stellar Parameters
Teff : 4932 | log g : 2.20 | vturb : 1.4 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
C | N/A | ... | -0.40 | ... | -1.96 | -0.28 | 6.47 | C |
O | N/A | -1.20 | 0.48 | ... | -1.02 | 0.66 | 7.67 | O |
Fe | N/A | -1.68 | ... | ... | -1.68 | ... | 5.82 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1999-09-27 | N/A | PHOENIXKPNO | 60000 | 100 | 4x1800 | N/A |
Oxygen Abundances in Metal-poor Stars
Stellar Parameters
Teff : 4900 | log g : 2.24 | vturb : 1.45 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
O I | N/A | ... | 0.61+-0.16 | 7.66+-0.16 | -1.03+-0.16 | 0.59+-0.16 | 7.66+-0.16 | O I |
Fe | N/A | -1.64 | ... | ... | -1.62 | ... | 5.88 | Fe |
Fe I | N/A | ... | ... | 5.89+-0.06 | -1.61+-0.06 | ... | 5.89+-0.06 | Fe I |
Fe II | N/A | ... | ... | 5.88+-0.07 | -1.62+-0.07 | ... | 5.88+-0.07 | Fe II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-09-29 | N/A | GECKOCFHT | 130000 | 190 | 900 | N/A |
ABUNDANCES AND KINEMATICS OF FIELD HALO AND DISK STARS. I. OBSERVATIONAL DATA AND ABUNDANCE ANALYSIS
Stellar Parameters
Teff : 4825 | log g : 2 | vturb : 1.45 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li I | N/A | ... | ... | 0.93 | -2.33 | -0.61 | 0.93 | Li I |
Na I | N/A | ... | -0.08 | ... | -1.73 | -0.01 | 4.51 | Na I |
Mg I | N/A | ... | 0.61 | ... | -1.15 | 0.57 | 6.45 | Mg I |
Al I | N/A | ... | 0.21 | ... | -1.51 | 0.21 | 4.94 | Al I |
Si I | N/A | ... | 0.48 | ... | -1.22 | 0.50 | 6.29 | Si I |
Ca I | N/A | ... | 0.41 | ... | -1.31 | 0.41 | 5.03 | Ca I |
Ti | N/A | ... | 0.32 | ... | -1.38 | 0.34 | 3.57 | Ti |
V I | N/A | ... | -0.05 | ... | -1.72 | 0.00 | 2.21 | V I |
Cr I | N/A | ... | -0.08 | ... | -1.79 | -0.07 | 3.85 | Cr I |
Fe | N/A | -1.74 | ... | ... | -1.72 | ... | 5.78 | Fe |
Ni I | N/A | ... | 0.02 | ... | -1.69 | 0.03 | 4.53 | Ni I |
Y II | N/A | ... | -0.08 | ... | -1.79 | -0.07 | 0.42 | Y II |
Zr II | N/A | ... | 0.27 | ... | -1.45 | 0.27 | 1.13 | Zr II |
Ba II | N/A | ... | 0.03 | ... | -1.76 | -0.04 | 0.42 | Ba II |
Eu II | N/A | ... | 0.51 | ... | -1.24 | 0.48 | -0.72 | Eu II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998-10-30 | N/A | LICKHAMILTON | 50000 | 90 | 1200 | N/A |
The Rise of the s-Process in the Galaxy
Stellar Parameters
Teff : 4870 | log g : 2.27 | vturb : 1.40 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
C | N/A | ... | -0.15 | ... | -1.68 | 0.03 | 6.75 | C |
Fe I | 10 | -1.71 | ... | ... | -1.71 | ... | 5.79 | Fe I |
Fe II | 7 | -1.68 | ... | ... | -1.68 | ... | 5.82 | Fe II |
La II | N/A | ... | ... | -0.42+-0.07 | -1.52+-0.07 | 0.19+-0.07 | -0.42+-0.07 | La II |
Eu II | N/A | ... | ... | -0.81+-0.03 | -1.33+-0.03 | 0.38+-0.03 | -0.81+-0.03 | Eu II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Spectroscopic Binaries, Velocity Jitter, and Rotation in Field Metal-poor Red Giant and Red Horizontal-Branch Stars
Stellar Parameters
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Fe | N/A | -1.65 | ... | ... | -1.65 | ... | 5.85 | Fe |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | 2445951.88220 | WYETH | N/A | N/A | N/A | 153.36+-0.44 |
N/A | 2446008.78363 | WYETH | N/A | N/A | N/A | 154.32+-0.52 |
N/A | 2446306.83512 | WYETH | N/A | N/A | N/A | 154.20+-0.58 |
N/A | 2446695.90478 | WYETH | N/A | N/A | N/A | 153.91+-1.01 |
N/A | 2447054.90212 | WYETH | N/A | N/A | N/A | 152.47+-0.62 |
N/A | 2447411.88173 | WYETH | N/A | N/A | N/A | 152.79+-0.73 |
N/A | 2447780.83274 | WYETH | N/A | N/A | N/A | 152.39+-0.47 |
N/A | 2448145.86194 | WYETH | N/A | N/A | N/A | 153.42+-0.63 |
N/A | 2448587.67691 | WYETH | N/A | N/A | N/A | 152.02+-0.59 |
N/A | 2449018.47147 | WYETH | N/A | N/A | N/A | 153.46+-0.65 |
N/A | 2450660.83758 | WYETH | N/A | N/A | N/A | 153.24+-0.52 |
Chemical Evolution of Zinc in the Galaxy
Stellar Parameters
Teff : 5010 | log g : 2.60 | vturb : 1.40 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Fe I | N/A | -1.47 | ... | ... | -1.52 | ... | 5.98 | Fe I |
Fe II | N/A | -1.47 | ... | ... | -1.52 | ... | 5.98 | Fe II |
Zn I | N/A | ... | -0.06+-0.1 | ... | -1.49+-0.1 | 0.03+-0.1 | 3.07+-0.1 | Zn I |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | OAO | 50000 | 220 | N/A | N/A |
THE UBIQUITY OF THE RAPID NEUTRON-CAPTURE PROCESS
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Fe | N/A | -1.71 | ... | ... | -1.71 | ... | 5.79 | Fe |
Zn I | N/A | ... | ... | 2.99 | -1.57 | 0.14 | 2.99 | Zn I |
Y II | N/A | ... | ... | 0.44 | -1.77 | -0.06 | 0.44 | Y II |
Pb I | N/A | ... | ... | <+0.50 | <-1.54 | <0.17 | <+0.50 | Pb I |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Sulphur abundances in halo giants from the [SI] line at 1082 nm and the SI triplet around 1045 nm
Stellar Parameters
Teff : 4900+-103 | log g : 2.24+-0.2 | vturb : 1.45+-0.5 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Si | N/A | ... | ... | 6.06 | -1.45 | 0.19 | 6.06 | Si |
S I | N/A | ... | ... | 6.03+-0.05 | -1.09+-0.05 | 0.55+-0.05 | 6.03+-0.05 | S I |
[S I] | N/A | ... | ... | 6.02 | -1.10 | 0.54 | 6.02 | [S I] |
Fe | N/A | -1.64+-0.09 | ... | ... | -1.64+-0.09 | ... | 5.86+-0.09 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-01-16 | N/A | VLTCRIRES | 80000 | 310-330 | 1920 | N/A |
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 4940+-40 | log g : 2.1+-0.2 | vturb : 1.5+-0.06 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li I | 1 | ... | ... | 1.07 | -2.19 | -0.49 | 1.07 | Li I |
CH | 1 | ... | 0.01+-0.25 | 6.62 | -1.81 | -0.11+-0.25 | 6.62 | CH |
NH | 1 | ... | -0.46+-0.36 | 5.55 | -2.28 | -0.58+-0.36 | 5.55 | NH |
O I | 4 | ... | 0.42+-0.15 | 7.40 | -1.29 | 0.41+-0.15 | 7.40 | O I |
Na I | 2 | ... | -0.10+-0.17 | 4.43 | -1.81 | -0.11+-0.17 | 4.43 | Na I |
Mg I | 4 | ... | 0.39+-0.18 | 6.29 | -1.31 | 0.39+-0.18 | 6.29 | Mg I |
Si I | 3 | ... | 0.43+-0.21 | 6.24 | -1.27 | 0.43+-0.21 | 6.24 | Si I |
K I | 1 | ... | 0.31+-0.24 | 3.64 | -1.39 | 0.31+-0.24 | 3.64 | K I |
Ca I | 10 | ... | 0.47+-0.24 | 5.11 | -1.23 | 0.47+-0.24 | 5.11 | Ca I |
Sc II | 4 | ... | 0.11+-0.15 | 1.44 | -1.71 | -0.01+-0.15 | 1.44 | Sc II |
Ti I | 15 | ... | 0.13+-0.15 | 3.38 | -1.57 | 0.13+-0.15 | 3.38 | Ti I |
Ti II | 17 | ... | 0.44+-0.15 | 3.57 | -1.38 | 0.32+-0.15 | 3.57 | Ti II |
V I | 1 | ... | -0.23+-0.24 | 2.00 | -1.93 | -0.23+-0.24 | 2.00 | V I |
V II | 2 | ... | 0.30+-0.25 | 2.42 | -1.51 | 0.19+-0.25 | 2.42 | V II |
Cr I | 8 | ... | -0.15+-0.14 | 3.79 | -1.85 | -0.15+-0.14 | 3.79 | Cr I |
Cr II | 3 | ... | 0.28+-0.15 | 4.11 | -1.53 | 0.17+-0.15 | 4.11 | Cr II |
Mn I | 3 | ... | -0.47+-0.14 | 3.26 | -2.17 | -0.47+-0.14 | 3.26 | Mn I |
Fe I | 88 | -1.70+-0.15 | ... | 5.80 | -1.70+-0.15 | ... | 5.80 | Fe I |
Fe II | 9 | -1.82+-0.15 | ... | 5.68 | -1.82+-0.15 | ... | 5.68 | Fe II |
Co I | 1 | ... | -0.31+-0.30 | 2.98 | -2.01 | -0.31+-0.30 | 2.98 | Co I |
Ni I | 9 | ... | -0.02+-0.17 | 4.50 | -1.72 | -0.02+-0.17 | 4.50 | Ni I |
Cu I | 1 | ... | -0.58+-0.14 | 1.91 | -2.28 | -0.58+-0.14 | 1.91 | Cu I |
Zn I | 2 | ... | 0.14+-0.14 | 3.00 | -1.56 | 0.14+-0.14 | 3.00 | Zn I |
Rb I | 1 | ... | <0.89 | <1.71 | <-0.65 | <1.05 | <1.71 | Rb I |
Sr II | 1 | ... | 0.26+-0.08 | 1.31 | -1.56 | 0.14+-0.08 | 1.31 | Sr II |
Y II | 5 | ... | -0.19+-0.15 | 0.20 | -2.01 | -0.31+-0.15 | 0.20 | Y II |
Zr II | 3 | ... | 0.35+-0.16 | 1.12 | -1.46 | 0.24+-0.16 | 1.12 | Zr II |
Nb II | 1 | ... | <1.02 | <0.66 | <-0.80 | <0.90 | <0.66 | Nb II |
Mo I | 1 | ... | 0.17+-0.17 | 0.35 | -1.53 | 0.17+-0.17 | 0.35 | Mo I |
Sn I | 1 | ... | <0.88 | <1.25 | <-0.82 | <0.88 | <1.25 | Sn I |
Ba II | 3 | ... | 0.20+-0.15 | 0.56 | -1.62 | 0.08+-0.15 | 0.56 | Ba II |
La II | 4 | ... | 0.09+-0.15 | -0.63 | -1.73 | -0.03+-0.15 | -0.63 | La II |
Ce II | 5 | ... | 0.10+-0.16 | -0.14 | -1.72 | -0.02+-0.16 | -0.14 | Ce II |
Pr II | 2 | ... | 0.37+-0.16 | -0.72 | -1.44 | 0.26+-0.16 | -0.72 | Pr II |
Nd II | 5 | ... | 0.27+-0.15 | -0.13 | -1.55 | 0.15+-0.15 | -0.13 | Nd II |
Sm II | 1 | ... | 0.31+-0.15 | -0.55 | -1.51 | 0.19+-0.15 | -0.55 | Sm II |
Eu II | 2 | ... | 0.33+-0.17 | -0.97 | -1.49 | 0.21+-0.17 | -0.97 | Eu II |
Gd II | 2 | ... | 0.48+-0.16 | -0.27 | -1.34 | 0.36+-0.16 | -0.27 | Gd II |
Dy II | 2 | ... | 0.34+-0.15 | -0.38 | -1.48 | 0.22+-0.15 | -0.38 | Dy II |
Er II | 3 | ... | 0.34+-0.17 | -0.55 | -1.47 | 0.23+-0.17 | -0.55 | Er II |
Tm II | 1 | ... | 0.38+-0.18 | -1.34 | -1.46 | 0.24+-0.18 | -1.34 | Tm II |
Yb II | 1 | ... | 0.21+-0.23 | -0.69 | -1.61 | 0.09+-0.23 | -0.69 | Yb II |
Hf II | 2 | ... | 0.59+-0.18 | -0.38 | -1.09 | 0.61+-0.18 | -0.38 | Hf II |
Pb I | 1 | ... | <0.45 | <0.79 | <-1.25 | <0.45 | <0.79 | Pb I |
Binary Parameters
Binarity | Negative |
Vrad | 153.7 |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2011-02-25-00:25 | 2455617.516 | MIKELCO | 41000 | 90-305 | 200 | 153.7 |