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• HG-WELS Bigger Picture and Goals
  ...(from Carlberg et al 2012), do we see a correlation between IR excess and Li like the de la Reza sample did?
  2 KB (338 words) - 22:31, 23 July 2014
• Pre-main sequence evolution
  ...ing H. They can (and do!) burn Li and D during these early phases, because Li and D are far easier to pull apart than it is to squish 2 Hs and 2 neutrons ...ady to burn H. I think some of the structure too comes from burning D and Li, but I've forgotten now if Iben has this in his models, and I can't find it
  5 KB (913 words) - 03:57, 2 October 2012
• Coherent ideas of what to do with these pieces
  *Li-rich giants project - extending to new samples, e.g., https://www.nature.co
  7 KB (1,086 words) - 17:04, 30 July 2024
• Working with the HG-WELS data
  ...catalog - much less biased set of giants assembled without regard to IR or Li, spanning range of vsini ...berg's private communication set of objects mentioned in the literature as Li rich (some of which subsequently vanished from de la reza's papers)
  31 KB (5,458 words) - 20:37, 28 August 2014
• Finding cluster members
  ...troscopy: high-res spectra can also tell you if the star still has lithum (Li burns so easily that only the youngest stars are thought to have any left)
  19 KB (3,216 words) - 23:02, 25 January 2024