G 15-13: 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	200	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	5082+-60
log g	4.61+-0.33
v_turb	0.00+-0.50

Chemical Abundances

Element	Nline	[X/H]	[X/Fe]	log-e
Li I	...	-0.83+-0.05	0.87+-0.05	0.33+-0.05
Fe	...	-1.70+-0.09	...	5.80+-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	2450595.273	KECKHIRES	48000	200	1800	219.7+-0.5

Binarity

Vrad	219.7+-0.5

Photometric data

V	12.325
B-V	0.755

Atmospheric data

T_eff	5082+-60
log g	4.61+-0.33
v_turb	0.00+-0.50

Chemical Abundances

Element	Nline	[X/H]	[X/Fe]	log-e
Na I	...	-2.32+-0.03	-0.60+-0.07	4.01+-0.03
Mg I	...	-1.55+-0.06	+0.16+-0.08	6.03+-0.06
Si	...	-1.54+-0.11	+0.18+-0.11	6.01+-0.11
Si I	...	-1.54+-0.10	0.18+-0.10	6.01+-0.10
Ca I	...	-1.52+-0.09	+0.20+-0.11	4.84+-0.09
Ti	...	-1.51+-0.08	+0.21+-0.08	3.51+-0.08
Ti I	...	-1.55+-0.07	0.17+-0.07	3.47+-0.07
Ti II	...	-1.47+-0.07	0.25+-0.07	3.55+-0.07
Cr	...	-1.70+-0.10	+0.02+-0.10	3.97+-0.10
Cr I	...	-1.73+-0.09	-0.01+-0.09	3.94+-0.09
Cr II	...	-1.54+-0.22	0.18+-0.22	4.13+-0.22
Fe	...	-1.72+-0.06	...	5.78+-0.06
Fe I	...	-1.69+-0.07	...	5.81+-0.07
Fe II	...	-1.75+-0.09	...	5.75+-0.09
Ni I	...	-1.87+-0.09	-0.16+-0.11	4.38+-0.09
Y II	...	-1.75+-0.04	-0.03+-0.07	0.49+-0.04
Ba II	...	-1.56+-0.05	+0.15+-0.08	0.57+-0.05

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