BD+24_1676: found in 8 paper(s).
Labels:
/P.E.Nissen et al.(2002)/
/E.Arnone et al.(2005)/
/A.Hosford et al.(2009)/
/D.K.Lai et al.(2008)/
/I.I.Ivans et al.(2003)/
/C.Charbonnel and F. Primas(2005)/
/A.M.Boesgaard et al.(2005)/
/A.Stephens and A. M. Boesgaard(2002)/
Find this object in SIMBAD
A0048
Get more information of this paper.
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
Atmospheric data
Teff | 6251 |
log g | 3.81 |
vturb | 1.5 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe | ... | -2.41 | ... | 5.09 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0075
Title | Mg abundances in metal-poor halo stars as a tracer of early Galactic mixing |
ADS | E.Arnone et al.,AAP, 430, 507, 2005 |
Authors | E. Arnone, S. G. Ryan, D. Argast, J. E. Norris, T. C. Beers |
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | ANGLO | 40000 | >100 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 6170 |
log g | 3.7+-0.2 |
vturb | 1.8+-0.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Mg I | ... | -2.28+-0.01 | 0.32+-0.01 | 5.30+-0.01 |
Ca I | ... | -2.21+-0.03 | 0.39+-0.03 | 4.15+-0.03 |
Ti I | ... | -2.07 | 0.53 | 2.95 |
Ti II | ... | -2.19 | 0.41 | 2.83 |
Cr I | ... | -2.72+-0.08 | -0.12+-0.08 | 2.95+-0.08 |
Fe I | ... | -2.60+-0.02 | ... | 4.90+-0.02 |
Fe II | ... | -2.60 | ... | 4.90 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0169
Title | Lithium abundances of halo dwarfs based on excitation temperature. I. Local thermodynamic equilibrium |
ADS | A.Hosford et al.,AAP, 493, 601, 2009 |
Authors | A. Hosford, S. G. Ryan, A. E. GarciaPerez, J. E. Norris, K. A. Olive |
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | ANGLO | 43000 | 100 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | 241142 |
Right Ascension | 072739 |
Photometric data
Atmospheric data
Teff | 6296+-55 |
log g | 4.47+-0.14 |
vturb | 1.20 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | 1.02+-0.009 | 3.55+-0.009 | 2.18+-0.009 |
Fe | ... | -2.53 | ... | 4.97 |
Fe I | ... | -2.60 | ... | 4.90 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0181
Title | Detailed Abundances for 28 Metal-poor Stars: Stellar Relics in the Milky Way |
ADS | D.K.Lai et al.,ApJ, 681, 1524, 2008 |
Authors | D. K. Lai, M. Bolte, J. A. Johnson, S. Lucatello |
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-10-07 | N/A | KECKHIRES | N/A | 288 | 3600 | -237.8+-0.2 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 6241+-100 |
log g | 3.81+-0.2 |
vturb | 1.6+-0.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -2.22+-0.21 | 0.41+-0.21 | 6.33+-0.21 |
N | ... | <-2.42 | <0.21 | <5.55 |
OH | ... | -1.98 | 0.65 | 6.89 |
Mg | ... | -2.26+-0.03 | 0.37+-0.03 | 5.32+-0.03 |
Si | ... | -2.46+-0.15 | 0.17+-0.15 | 5.09+-0.15 |
Ca | ... | -2.18+-0.03 | 0.45+-0.03 | 4.18+-0.03 |
Sc II | ... | -2.43+-0.05 | 0.20+-0.05 | 0.74+-0.05 |
Ti I | ... | -2.08+-0.03 | 0.55+-0.03 | 2.94+-0.03 |
Ti II | ... | -2.18+-0.06 | 0.45+-0.06 | 2.84+-0.06 |
V II | ... | -2.43+-0.09 | 0.20+-0.09 | 1.57+-0.09 |
Cr I | ... | -2.76+-0.04 | -0.13+-0.04 | 2.91+-0.04 |
Cr II | ... | -2.72+-0.08 | -0.09+-0.08 | 2.95+-0.08 |
Mn I | ... | -3.06+-0.09 | -0.43+-0.09 | 2.33+-0.09 |
Mn II | ... | -2.93+-0.06 | -0.30+-0.06 | 2.46+-0.06 |
Fe I | ... | -2.63+-0.08 | ... | 4.87+-0.08 |
Fe II | ... | -2.60+-0.06 | ... | 4.90+-0.06 |
Co | ... | -2.28+-0.06 | 0.35+-0.06 | 2.64+-0.06 |
Ni | ... | -2.60+-0.04 | 0.03+-0.04 | 3.65+-0.04 |
Cu | ... | -3.46+-0.06 | -0.83+-0.06 | 0.75+-0.06 |
Zn | ... | -2.43+-0.18 | 0.20+-0.18 | 2.17+-0.18 |
Sr II | ... | -2.68+-0.08 | -0.05+-0.08 | 0.29+-0.08 |
Y II | ... | -2.75+-0.06 | -0.12+-0.06 | -0.51+-0.06 |
Zr II | ... | -2.32+-0.09 | 0.31+-0.09 | 0.28+-0.09 |
Ba II | ... | -2.96+-0.09 | -0.33+-0.09 | -0.83+-0.09 |
Eu II | ... | <-2.04 | <0.59 | <-1.53 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0188
Title | Chemical Substructure in the Milky Way Halo: A New Population of Old Stars |
ADS | I.I.Ivans et al.,ApJ, 592, 906, 2003 |
Authors | I. I. Ivans, C. Sneden, C. R. James, G. W. Preston, J. P. Fulbright, P. A. Hoflich, B. W. Carney, J. C. Wheeler |
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1997-11-09 | N/A | MAYALLKPNO | 28000 | 90-150 | 3600 | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | +240510 |
Right Ascension | 073041.3 |
Photometric data
V | 10.80 |
B-V | 0.35 |
EB-V | 0.05 |
Atmospheric data
Teff | 6250 |
log g | 3.45 |
vturb | 1.20 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | 1.29 | 3.79 | 2.45 |
O I | ... | -1.63+-0.16 | +0.87+-0.16 | 7.24+-0.16 |
Na I | ... | -2.70+-0.05 | -0.20+-0.05 | 3.63+-0.05 |
Mg I | ... | -2.01+-0.24 | +0.49+-0.24 | 5.57+-0.24 |
Al I | ... | <-1.42 | <+1.08 | <5.05 |
Si I | ... | <-1.72 | <+0.78 | <5.83 |
K I | ... | <-1.63 | <+0.87 | <3.49 |
Ca I | ... | -2.07+-0.09 | +0.43+-0.09 | 4.29+-0.09 |
Sc I | ... | <0.81 | <+3.31 | <3.98 |
Sc II | ... | -2.13+-0.14 | +0.37+-0.14 | 1.04+-0.14 |
Ti I | ... | -2.04+-0.09 | +0.46+-0.09 | 2.98+-0.09 |
Ti II | ... | -2.16+-0.15 | +0.34+-0.15 | 2.86+-0.15 |
V I | ... | <-0.34 | <+2.16 | <3.66 |
Cr I | ... | -2.48+-0.27 | +0.02+-0.27 | 3.19+-0.27 |
Cr II | ... | <-1.63 | <+0.87 | <4.04 |
Mn I | ... | -2.09 | +0.41 | 3.30 |
Fe I | ... | -2.50+-0.20 | ... | 5.00+-0.20 |
Fe II | ... | -2.48+-0.15 | ... | 5.02+-0.15 |
Ni I | ... | -2.20+-0.19 | +0.30+-0.19 | 4.05+-0.19 |
Cu I | ... | -1.89 | +0.61 | 2.32 |
Y II | ... | -2.33 | +0.17 | -0.09 |
Ba II | ... | -2.99+-0.04 | -0.49+-0.04 | -0.86+-0.04 |
La II | ... | <-0.36 | <+2.14 | <0.81 |
Eu II | ... | <-0.29 | <+2.21 | <0.22 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0191
Get more information of this paper.
Basic Informations
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | 24.08618 |
Right Ascension | 112.67194 |
Photometric data
V | 10.8 |
B-V | 0.35 |
EB-V | 0.057 |
Atmospheric data
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | 1.00+0.078-0.094 | 3.65+0.078-0.094 | 2.159+0.078-0.094 |
Fe | ... | -2.65+-0.060 | ... | 4.85+-0.060 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0193
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | KECKHIRES | 48000 | 120 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 6136+-71 |
log g | 3.54+-0.37 |
vturb | 1.59+-0.16 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | 1.01+-0.06 | 3.57+-0.06 | 2.17+-0.06 |
Fe | ... | -2.56+-0.07 | ... | 4.94+-0.07 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0199
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | 2450820.346 | KECKHIRES | 48000 | 120 | 300 | -237.7+-0.6 |
Binarity
Photometric data
Atmospheric data
Teff | 6136+-71 |
log g | 3.54+-0.37 |
vturb | 1.59+-0.16 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Mg I | ... | -2.02+-0.16 | +0.53+-0.17 | 5.56+-0.16 |
Ca I | ... | -2.18+-0.06 | +0.37+-0.09 | 4.18+-0.06 |
Ti | ... | -2.09+-0.09 | +0.46+-0.09 | 2.93+-0.09 |
Ti I | ... | -2.10+-0.08 | 0.45+-0.08 | 2.92+-0.08 |
Ti II | ... | -2.08+-0.10 | 0.47+-0.10 | 2.94+-0.10 |
Cr | ... | -2.55+-0.16 | +0.00+-0.16 | 3.12+-0.16 |
Cr I | ... | -2.54+-0.14 | 0.01+-0.14 | 3.13+-0.14 |
Fe | ... | -2.55+-0.06 | ... | 4.95+-0.06 |
Fe I | ... | -2.55+-0.07 | ... | 4.95+-0.07 |
Fe II | ... | -2.54+-0.13 | ... | 4.96+-0.13 |
Ni I | ... | -2.45+-0.16 | +0.10+-0.17 | 3.80+-0.16 |
Ba II | ... | -2.96+-0.13 | -0.42+-0.15 | -0.83+-0.13 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)