Abundances in bulge stars from high-resolution, near-IR spectra - I. The CNO elements observed during the science verification of CRIRES at VLT

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Table 1:

Log of our observations. The stars are taken from Arp (1965).
Star	RA	dec	H	$t_{\rm exp}$	SNR
Arp 4203	18 03 23.6	-30 01 59	9.2	200 s	80
Arp 4329	18 03 28.4	-29 58 42	11.1	1800 s	95
Arp 1322	18 03 49.4	-30 01 54	10.3	600 s	110

Source LaTeX | All tables | In the text

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