HR5447

HR5447

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	-0.47	...	...	-0.47	...	7.03	Fe I
Fe II	N/A	-0.56	...	...	-0.56	...	6.94	Fe II
La II	N/A	...	...	0.79	-0.31	0.16	0.79	La II
Eu II	N/A	...	...	0.11	-0.41	0.06	0.11	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	...	0.09	...	-0.23	0.18	6.01	Na
Mg	N/A	...	0.04	...	-0.39	0.02	7.21	Mg
Ca	N/A	...	0.05	...	-0.34	0.07	6.00	Ca
Fe	N/A	-0.41	...	...	-0.41	...	7.09	Fe
Ni	N/A	...	0.01	...	-0.37	0.04	5.85	Ni
Y	N/A	...	0.17	...	-0.21	0.20	2.00	Y
Ba	N/A	...	-0.04	...	-0.50	-0.09	1.68	Ba