G 144-28: 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	140	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	5310+-65
log g	4.19+-0.39
v_turb	1.16+-0.12

Chemical Abundances

Element	Nline	[X/H]	[X/Fe]	log-e
Li I	...	0.35+-0.05	2.45+-0.05	1.51+-0.05
Fe	...	-2.10+-0.06	...	5.40+-0.06

: 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	2451067.433	KECKHIRES	48000	140	1800	-13.2+-0.7

Binarity

Vrad	-13.2+-0.7

Photometric data

V	12.930
B-V	0.630

Atmospheric data

T_eff	5310+-65
log g	4.19+-0.39
v_turb	1.16+-0.12

Chemical Abundances

Element	Nline	[X/H]	[X/Fe]	log-e
Na I	...	-1.94+-0.17	+0.20+-0.17	4.39+-0.17
Mg I	...	-1.78+-0.16	+0.36+-0.17	5.80+-0.16
Si	...	-1.78+-0.17	+0.36+-0.17	5.77+-0.17
Si I	...	-1.78+-0.16	0.36+-0.16	5.77+-0.16
Ca I	...	-1.78+-0.11	+0.36+-0.12	4.58+-0.11
Ti	...	-1.86+-0.08	+0.28+-0.08	3.16+-0.08
Ti I	...	-1.91+-0.08	0.23+-0.08	3.11+-0.08
Ti II	...	-1.81+-0.07	0.33+-0.07	3.21+-0.07
Cr	...	-2.14+-0.08	-0.00+-0.08	3.53+-0.08
Cr I	...	-2.17+-0.06	-0.03+-0.06	3.50+-0.06
Cr II	...	-2.02+-0.12	0.12+-0.12	3.65+-0.12
Fe	...	-2.14+-0.05	...	5.36+-0.05
Fe I	...	-2.09+-0.07	...	5.41+-0.07
Fe II	...	-2.21+-0.09	...	5.29+-0.09
Ni I	...	-2.11+-0.10	+0.02+-0.12	4.14+-0.10
Y II	...	-2.35+-0.19	-0.21+-0.19	-0.11+-0.19
Ba II	...	-2.23+-0.06	-0.09+-0.08	-0.10+-0.06

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