G 116-53: found in 2 paper(s).

Labels:

/A.M.Boesgaard et al.(2005)/ /A.Stephens and A. M. Boesgaard(2002)/

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A0193

Title	Lithium and Lithium Depletion in Halo Stars on Extreme Orbits
ADS	A.M.Boesgaard et al.,ApJ, 633, 398, 2005
Authors	A. M. Boesgaard, A. Stephens, C. P. Deliyannis

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Basic Informations

Observation Date	JD	Facility	Resolution	S/N	Exposure Time	Vrad
	N/A	KECKHIRES	48000	100	N/A	N/A

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

Atmospheric data

T_eff	5732+-72
log g	4.45+-0.27
v_turb	0.40+-0.23

Chemical Abundances

Element	Nline	[X/H]	[X/Fe]	log-e
Li I	...	0.68+-0.06	1.65+-0.06	1.84+-0.06
Fe	...	-0.97+-0.09	...	6.53+-0.09

: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)

A0199

Title	ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS
ADS	A.Stephens et al.,AJ, 123, 1647, 2002
Authors	A. Stephens, A. M. Boesgaard

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Basic Informations

Observation Date	JD	Facility	Resolution	S/N	Exposure Time	Vrad
N/A	2450820.569	KECKHIRES	48000	100	2000	-112.4+-1.7

Binarity

Vrad	-112.4+-1.7

Photometric data

V	12.985
B-V	0.550

Atmospheric data

T_eff	5732+-72
log g	4.45+-0.27
v_turb	0.40+-0.23

Chemical Abundances

Element	Nline	[X/H]	[X/Fe]	log-e
Na I	...	-1.29+-0.15	-0.27+-0.16	5.04+-0.15
Mg I	...	-0.86+-0.20	+0.16+-0.20	6.72+-0.20
Si	...	-0.91+-0.09	+0.12+-0.09	6.64+-0.09
Si I	...	-0.91+-0.08	0.12+-0.08	6.64+-0.08
Si II	...	-0.86+-0.16	0.17+-0.16	6.69+-0.16
Ca I	...	-0.87+-0.09	+0.16+-0.10	5.49+-0.09
Ti	...	-0.84+-0.10	+0.19+-0.10	4.18+-0.10
Ti I	...	-0.89+-0.11	0.14+-0.11	4.13+-0.11
Ti II	...	-0.78+-0.12	0.25+-0.12	4.24+-0.12
Cr	...	-1.03+-0.08	+0.00+-0.08	4.64+-0.08
Cr I	...	-1.03+-0.07	0.00+-0.07	4.64+-0.07
Cr II	...	-1.00+-0.13	0.03+-0.13	4.67+-0.13
Fe	...	-1.03+-0.05	...	6.47+-0.05
Fe I	...	-0.96+-0.08	...	6.54+-0.08
Fe II	...	-1.07+-0.07	...	6.43+-0.07
Ni I	...	-1.12+-0.13	-0.09+-0.14	5.13+-0.13
Y II	...	-1.12+-0.04	-0.10+-0.07	1.12+-0.04
Ba II	...	-0.81+-0.06	+0.21+-0.08	1.32+-0.06

: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)