Exploració per autor "Iliadis, Christian"

Ara es mostren els items 1-5 de 5

    • Hydrodynamic simulations of classical novae: accretion onto CO white dwarfs as SN Ia progenitors 

      Starrfield, Sumner; Bose, M; Iliadis, Christian; Hix, W. R.; Woodward, C; Wagner, R; José Pont, Jordi; Hernanz Carbó, Margarita (PoS - Proceedings of Science, 2018)
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    • Hydrogen burning of 29Si and its impact on presolar stardust grains from classical novae 

      Downen, Lori N.; Iliadis, Christian; Champagne, Art; Clegg, Thomas; Coc, Alain; José Pont, Jordi (Institute of Physics (IOP), 2022-04-01)
      Article
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      Presolar stardust grains found in primitive meteorites are believed to retain the isotopic composition of stellar outflows at the time of grain condensation. Therefore, laboratory measurements of their isotopic ratios ...

    • Mean proton and alpha-particle reduced widths of the Porter-Thomas distribution and astrophysical applications 

      Pogrebnyak, I.; Howard, C.; Iliadis, Christian; Longland, Richard Leigh; Mitchell, G.E. (2013-07)
      Article
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      The Porter-Thomas distribution is a key prediction of the Gaussian orthogonal ensemble in random matrix theory. It is routinely used to provide a measure for the number of levels that are missing in a given resonance ...

    • 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
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      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
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      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 ...