HR4657

HR4657

taken from 2 paper(s):

/J.Simmerer et al.(2004)/ /K.A.Venn et al.(2004)/

J.Simmerer et al.,ApJ, 617, 1091, 2004(ADS)

The Rise of the s-Process in the Galaxy

Chemical Abundances

		Original Data			Converted Data Asplund et al. (2009)
Element	Nline	[X/H]	[X/Fe]	log-e	[X/H]	[X/Fe]	log-e	Element
Fe I	N/A	-0.76	...	...	-0.76	...	6.74	Fe I
Fe II	N/A	-0.87	...	...	-0.87	...	6.63	Fe II
La II	N/A	...	...	0.24	-0.86	-0.10	0.24	La II
Eu II	N/A	...	...	-0.05	-0.57	0.19	-0.05	Eu II

Position

Observing Log

Date of Observation	JD	Facility	Resolution	S/N	Exposure Time	Vrad
	N/A	MCDONALD	60000	100	N/A	N/A

K.A.Venn et al.,AJ, 128, 1177, 2004(ADS)

Stellar Chemical Signatures and Hierarchical Galaxy Formation

Chemical Abundances

		Original Data			Converted Data Asplund et al. (2009)
Element	Nline	[X/H]	[X/Fe]	log-e	[X/H]	[X/Fe]	log-e	Element
Na	N/A	...	0.12	...	-0.49	0.21	5.75	Na
Mg	N/A	...	0.34	...	-0.38	0.32	7.22	Mg
Ca	N/A	...	0.19	...	-0.49	0.21	5.85	Ca
Ti	N/A	...	0.32	...	-0.31	0.39	4.64	Ti
Fe	N/A	-0.7	...	...	-0.70	...	6.80	Fe
Ni	N/A	...	0.06	...	-0.61	0.09	5.61	Ni
Y	N/A	...	0.01	...	-0.66	0.04	1.55	Y
Ba	N/A	...	-0.32	...	-1.07	-0.37	1.11	Ba
Eu	N/A	...	0.24	...	-0.47	0.23	0.05	Eu