HR2601

HR2601

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	-0.61	...	...	-0.61	...	6.89	Fe I
Fe II	N/A	-0.7	...	...	-0.70	...	6.80	Fe II
La II	N/A	...	...	0.71	-0.39	0.22	0.71	La 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	...	0.02	...	-0.45	0.11	5.79	Na
Mg	N/A	...	0.24	...	-0.34	0.22	7.26	Mg
Ca	N/A	...	-0.01	...	-0.55	0.01	5.79	Ca
Ti	N/A	...	0.26	...	-0.23	0.33	4.72	Ti
Fe	N/A	-0.56	...	...	-0.56	...	6.94	Fe
Ni	N/A	...	0.05	...	-0.48	0.08	5.74	Ni
Y	N/A	...	0.07	...	-0.46	0.10	1.75	Y
Ba	N/A	...	-0.36	...	-0.97	-0.41	1.21	Ba