This from the IAU: COMET 17P/HOLMES H. Kobayashi, H. Kawakita, and A. Nishikoji, Kyoto Sangyo University, report that they have obtained low-dispersion spectra of comet 17P on Oct. 24.58 and 25.46 UT with a 28-cm telescope (+ F2SPEC spectrograph; range 380-750 nm, resolution 900 at 600 nm). The comet's spectrum on Oct. 24.58 was dominated by reflected sunlight, and there were no significant emission bands and lines visible. The Oct. 25.46 spectrum was still dominated by reflected sunlight, but emission bands and lines (CN and C_2 bands, as well as [O I] emission lines) appeared in the spectrum. The authors speculate that this delay in the visibility of emission might be at least partly caused by sublimation from icy grains ejected at the outburst. Paul Knauth School of Earth and Space Exploration Arizona State University Tempe, AZ 85287-1404 480-965-2867 (voice) 480-965-8102 (Fax) http://www.public.asu.edu/~iaclpk/ -- Binary/unsupported file stripped by Ecartis -- -- Type: application/ms-tnef -- File: winmail.dat -- See message header for info on list archives or unsubscribing, and please send personal replies to the author, not the list.