G 31-26: 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	145	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	5546+-75
log g	4.50+-0.46
v_turb	0.35+-0.23

Chemical Abundances

Element	Nline	[X/H]	[X/Fe]	log-e
Li I	...	0.43+-0.05	1.72+-0.05	1.59+-0.05
Fe	...	-1.29+-0.07	...	6.21+-0.07

: 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	2451067.531	KECKHIRES	48000	145	900	-215.6+-0.7

Binarity

Vrad	-215.6+-0.7

Photometric data

V	12.170
B-V	0.630

Atmospheric data

T_eff	5546+-75
log g	4.50+-0.46
v_turb	0.35+-0.23

Chemical Abundances

Element	Nline	[X/H]	[X/Fe]	log-e
Na I	...	-1.60+-0.16	-0.28+-0.17	4.73+-0.16
Mg I	...	-1.03+-0.05	+0.28+-0.08	6.55+-0.05
Si	...	-1.06+-0.08	+0.26+-0.08	6.49+-0.08
Si I	...	-1.06+-0.06	0.26+-0.06	6.49+-0.06
Ca I	...	-1.08+-0.09	+0.23+-0.11	5.28+-0.09
Ti	...	-1.08+-0.11	+0.24+-0.11	3.94+-0.11
Ti I	...	-1.13+-0.14	0.19+-0.14	3.89+-0.14
Ti II	...	-1.03+-0.12	0.29+-0.12	3.99+-0.12
Cr	...	-1.29+-0.08	+0.03+-0.08	4.38+-0.08
Cr I	...	-1.33+-0.07	-0.01+-0.07	4.34+-0.07
Cr II	...	-1.16+-0.12	0.16+-0.12	4.51+-0.12
Fe	...	-1.32+-0.05	...	6.18+-0.05
Fe I	...	-1.28+-0.07	...	6.22+-0.07
Fe II	...	-1.35+-0.07	...	6.15+-0.07
Ni I	...	-1.41+-0.14	-0.09+-0.14	4.84+-0.14
Y II	...	-1.41+-0.08	-0.09+-0.09	0.83+-0.08
Ba II	...	-1.24+-0.11	+0.08+-0.12	0.89+-0.11

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