Thanks for showing us that spectrum (and taking it, Keith!). This is a completely bland solar spectrum. If there were any emission to be detected visually, there would have to be a big broad C2 emission band around 5100A, just right of H-beta in Keith's spectrum. The yellowish color that everyone has been seeing is indicative of a straight reflection spectrum; you'd expect reports of turquoise-blue/green if the comet was gassy. This is consistent also with the outburst being basically a lot of dust coming from the comet; if it was a gassy event, I'm pretty sure the light distribution would be more nearly 1/radius (falling off smoothly in brightness) rather than having the more-or-less well-defined shells like we're seeing. \Brian -- See message header for info on list archives or unsubscribing, and please send personal replies to the author, not the list.