Chemical abundances of 11 bulge stars from high-resolution, near-IR spectra

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Table 1:

Account of our observations.
Star^a	RA (J2000)	Dec (J2000)	H	$t^b_{\rm integration}$	S/N
				[s]
B3-b1	18 08 15.8	-25 42 10	11.3	2400	60
B3-b7	18 09 16.9	-25 49 28	11.6	4200	40
B3-b8	18 08 24.6	-25 48 44	11.9	3840	90
BW-b6	18 04 45.1	-29 48 52	11.9	3840	60
BW-f6	18 04 56.1	-29 48 59	12.0	4800	90
B6-f1	18 10 04.5	-31 41 45	11.9	1920	50
B6-b8	18 09 55.9	-31 45 46	11.9	3840	60
B6-f7	18 03 52.3	-31 46 42	11.9	1920	50
Arp 4203	18 03 23.6	-30 01 59	9.2	200	80
Arp 4329	18 03 28.4	-29 58 42	11.1	1800	95
Arp 1322	18 03 49.4	-30 01 54	10.3	600	110

^a The designation of the stars is adopted from Lecureur et al. (2007); ^b the total integration times are given by NDIT $\times$ DIT $\times$ NEXP $\times$ NABCYCLES $\times$ 2, see the CRIRES User's manual at http://www.eso.org/sci/facilities/paranal/instruments/crires/doc/

Source LaTeX | All tables | In the text

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