G 88-42: 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	90	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	5192+-62
log g	4.20+-0.41
v_turb	0.00+-0.50

Chemical Abundances

Element	Nline	[X/H]	[X/Fe]	log-e
Li I	...	-0.08+-0.05	1.65+-0.05	1.08+-0.05
Fe	...	-1.73+-0.10	...	5.77+-0.10

: 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	2450820.352	KECKHIRES	48000	90	2700	391.7+-0.7
N/A	2450820.392	KECKHIRES	48000	90	2400	391.7+-0.7

Binarity

Vrad	391.7+-0.7

Photometric data

V	14.380
B-V	0.645

Atmospheric data

T_eff	5192+-62
log g	4.20+-0.41
v_turb	0.00+-0.50

Chemical Abundances

Element	Nline	[X/H]	[X/Fe]	log-e
Na I	...	-2.24+-0.08	-0.46+-0.10	4.09+-0.08
Mg I	...	-1.64+-0.16	+0.14+-0.17	5.94+-0.16
Si	...	-1.54+-0.09	+0.24+-0.09	6.01+-0.09
Si I	...	-1.54+-0.07	0.24+-0.07	6.01+-0.07
Ca I	...	-1.52+-0.12	+0.25+-0.14	4.84+-0.12
Ti	...	-1.68+-0.10	+0.10+-0.10	3.34+-0.10
Ti I	...	-1.70+-0.08	0.08+-0.08	3.32+-0.08
Ti II	...	-1.58+-0.16	0.20+-0.16	3.44+-0.16
Cr	...	-1.82+-0.09	-0.04+-0.09	3.85+-0.09
Cr I	...	-1.84+-0.07	-0.06+-0.07	3.83+-0.07
Cr II	...	-1.71+-0.18	0.07+-0.18	3.96+-0.18
Fe	...	-1.78+-0.07	...	5.72+-0.07
Fe I	...	-1.73+-0.08	...	5.77+-0.08
Fe II	...	-1.85+-0.10	...	5.65+-0.10
Ni I	...	-1.94+-0.13	-0.16+-0.15	4.31+-0.13
Y II	...	-2.28+-0.35	-0.50+-0.36	-0.04+-0.35
Ba II	...	-1.80+-0.06	-0.02+-0.09	0.33+-0.06

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