• On presolar stardust grains from CO classical novae 

      Iliadis, Christian; Downen, Lori N.; José Pont, Jordi; Nittler, Larry R.; Starrfield, Sumner (Institute of Physics (IOP), 2018-03-10)
      Article
      Accés obert
      About 30%–40% of classical novae produce dust 20–100 days after the outburst, but no presolar stardust grains from classical novae have been unambiguously identified yet. Although several studies claimed a nova paternity ...
    • Reaction rates for the s-process neutron source Ne-22+alpha 

      Longland, Richard Leigh; Iliadis, Christian; Karakas, A.I. (2012-06-25)
      Article
      Accés obert
      The 22Ne(α, n)25Mg reaction is an important source of neutrons for the s-process. In massive stars responsible for the weak component of the s-process, 22Ne(α, n)25Mg is the dominant source of neutrons, both during core ...