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Published online by Cambridge University Press: 25 April 2016
Wollman et al. (32.155.001) present high-resolution 2 um spectra of three red giant stars in the core of the Galaxy. The properties of 0H/IR stars were studied by Baud et al. (29.131.023), Olnon et al. (29.155.032), Habing et al. (34.155.048), and Baud (34.155.042). Vanderspeck and Ricker (34.041.001) determined absolute coordinates for 19 stars within 2’ of the galactic center for epoch 1958.3 and 1976.3 and calculated their proper motions. Mould (33.155.013) obtained the radial-velocity dispersion for M stars in the nuclear bulge.