Exploració per autor "Iliadis, Christian"
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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
Accés obertPresolar 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
Accés obertThe 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
Accés obertAbout 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 obertThe 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 ...