Mn, Cu, and Zn abundances in barium stars and their correlations with neutron capture elements

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Table 2

Lines, equivalent widths, and abundances.

Star	El	λ	χ _ex	log gf	Ref.	EW	log ϵ	[X/Fe]
		(Å)	(eV)			(mÅ)

HD 9362^*	Li I^**	6707.760	0.000	0.171	1	...	–0.34	...
HD 9362^*	Li I^**	6707.910	0.000	–0.299	2	...	–0.34	...
HD 9362^*	Li I^**	6708.087	0.000	0.000	3	...	–0.34	...
HD 9362^*	C	4295.000^a	...	...	...	...	8.16	–0.02
HD 9362^*	C	5135.600^b	...	...	...	...	8.19	0.01

Notes. Abundances of Mn for barium stars from Allen & Barbuy (2006a) are shown starting on line 1541. Note that HD 2454 is HR 107 in Allen & Barbuy (2006a). The full table is only available at the CDS. < indicates an upper limit. The gf-values sources are given below.

^(*)

indicates stars that were considered to be normal instead of barium stars by Smiljanic et al. (2007), and the well-known giant ϵ Vir (HD 113226), used by them as reference star;

^(**)

indicates multiple line;

^(a)

representative line for CH (G band);

^(b)

representative line for C₂;

^(c)

representative line for CN.

References. (1) McWilliam & Rich (1994); (2) NIST; (3) Barbuy et al. (1999); (4) Allende Prieto et al. (2001); (5) Lambert (1978); (6) Bielski (1975); (7) Biémont & Godefroid (1980); (8) Gratton & Sneden (1994); (9) Hannaford et al. (1982); (10) Hannaford & Lowe (1983); (11) Biémont et al. (1981); (12) Thévenin (1990); (13) Thévenin (1989); (14) Smith et al. (2000); (15) VALD; (16) McWilliam (1998); (17) Rutten (1978); (18) Lawler et al. (2001a); (19) Palmeri et al. (2000); (20) Goly et al. (1991); (21) Lage & Whaling (1976); (22) Hartog et al. (2003); (23) Maier & Whaling (1977); (24) Sneden et al. (1996); (25) Biémont et al. (1989); (26) Lawler et al. (2001b); (27) Bergstrom et al. (1988); (28) Corliss & Bozman (1962); (29) average between Kusz (1992) and Biémont & Lowe (1993); (30) Biémont et al. (2000); “SUN” indicates log gf obtained through fits on the solar spectrum.

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