tag:blogger.com,1999:blog-20092824.post6323827551930026685..comments2024-01-30T19:45:36.648+11:00Comments on Lounge of the Lab Lemming: Rare Earth Revelry: Week -1C W Mageehttp://www.blogger.com/profile/09706100504739548720noreply@blogger.comBlogger3125tag:blogger.com,1999:blog-20092824.post-12703821678803530202010-12-01T11:26:22.072+11:002010-12-01T11:26:22.072+11:00To make sure we use the right terminology: the &qu...To make sure we use the right terminology: the "s" in the s-process is for "slow" not for "star".amengonihttps://www.blogger.com/profile/03275954536805563587noreply@blogger.comtag:blogger.com,1999:blog-20092824.post-61084783540773507202010-11-23T04:04:14.140+11:002010-11-23T04:04:14.140+11:00Very interesting! I didn't know about the S-pr...Very interesting! I didn't know about the S-process, and it's cool how they could confirm the SiC origin with the Nd isotope ratios.<br /><br />Knowing that a lot of elements are created in large old boiling stars, I wonder how much of the chemistry in interstellar clouds happens near those stars, rather than post-supernova? Someone probably knows the answer by now, but I don't know Chris Phoenixhttps://www.blogger.com/profile/13368959552769808835noreply@blogger.comtag:blogger.com,1999:blog-20092824.post-68477045479063606972010-11-21T08:09:32.535+11:002010-11-21T08:09:32.535+11:00Thanks for doing this!Thanks for doing this!Judithnoreply@blogger.com