Non-standard s-process in low metallicity massive rotating stars
A&A, 538 (2012) L2
Published online: 2012-01-31
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https://doi.org/10.3847/1538-4357/aa8c74
Testing a one-dimensional prescription of dynamical shear mixing with a two-dimensional hydrodynamic simulation
P. V. F. Edelmann, F. K. Röpke, R. Hirschi, C. Georgy and S. JonesAstronomy & Astrophysics 604 A25 (2017)
https://doi.org/10.1051/0004-6361/201629873
Pre-supernova mixing in CEMP-no source stars
Arthur Choplin, Sylvia Ekström, Georges Meynet, et al.Astronomy & Astrophysics 605 A63 (2017)
https://doi.org/10.1051/0004-6361/201630182
GALACTIC CHEMICAL EVOLUTION: THE IMPACT OF THE 13C-POCKET STRUCTURE ON THE s-PROCESS DISTRIBUTION
S. Bisterzo, C. Travaglio, M. Wiescher, F. Käppeler and R. GallinoThe Astrophysical Journal 835 (1) 97 (2017)
https://doi.org/10.3847/1538-4357/835/1/97
THE ORIGIN OF THE HEAVIEST METALS IN MOST ULTRA-FAINT DWARF GALAXIES
Ian U. RoedererThe Astrophysical Journal 835 (1) 23 (2017)
https://doi.org/10.3847/1538-4357/835/1/23
The Intermediate r-process in Core-collapse Supernovae Driven by the Magneto-rotational Instability
N. Nishimura (西村信哉), H. Sawai (澤井秀朋), T. Takiwaki (滝脇知也), S. Yamada (山田章一) and F.-K. ThielemannThe Astrophysical Journal Letters 836 (2) L21 (2017)
https://doi.org/10.3847/2041-8213/aa5dee
Something borrowed, something blue: The nature of blue metal-poor stars inferred from their colours and chemical abundances
C. J. Hansen, P. Jofré, A. Koch, A. McWilliam and C. S. SnedenAstronomy & Astrophysics 598 A54 (2017)
https://doi.org/10.1051/0004-6361/201629628
Are some CEMP-s stars the daughters of spinstars?
Arthur Choplin, Raphael Hirschi, Georges Meynet and Sylvia EkströmAstronomy & Astrophysics 607 L3 (2017)
https://doi.org/10.1051/0004-6361/201731948
Handbook of Supernovae
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https://doi.org/10.1007/978-3-319-20794-0_82-1
Handbook of Supernovae
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https://doi.org/10.1007/978-3-319-21846-5_82
Uncertainties in s-process nucleosynthesis in massive stars determined by Monte Carlo variations
N. Nishimura (西村信哉), R. Hirschi, T. Rauscher, A. St. J. Murphy and G. CescuttiMonthly Notices of the Royal Astronomical Society 469 (2) 1752 (2017)
https://doi.org/10.1093/mnras/stx696
A Chemical Signature from Fast-rotating Low-metallicity Massive Stars: ROA 276 in ω Centauri*
David Yong, John E. Norris, Gary S. Da Costa, Laura M. Stanford, Amanda I. Karakas, Luke J. Shingles, Raphael Hirschi and Marco PignatariThe Astrophysical Journal 837 (2) 176 (2017)
https://doi.org/10.3847/1538-4357/aa6250
Does the chemical signature of TYC 8442–1036–1 originate from a rotating massive star that died in a faint explosion?
G. Cescutti, M. Valentini, P. François, et al.Astronomy & Astrophysics 595 A91 (2016)
https://doi.org/10.1051/0004-6361/201629106