0435756 - ÚJF 2015 RIV US eng C - Konferenční příspěvek (zahraniční konf.)
Sergi, M. L. - Spitaleri, C. - Pizzone, R. G. - Burjan, Václav - Cherubini, S. - Gulino, M. - Hons, Zdeněk - Kroha, Václav - La Cognata, M. - Lamia, L. … celkem 21 autorů
The O-17(p,alpha)N-14 reaction measurement via the Trojan Horse Method and its application to O-17 nucleosynthesis.
AIP Conference Proceedings. Vol. 1594. Melville: American Institute of Physics, 2014, s. 201-205. ISBN 978-0-7354-1228-6. ISSN 0094-243X.
[12th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG). Tsukuba (JP), 18.11.2013-21.11.2013]
Grant CEP: GA MŠMT(CZ) LH11001; GA MŠMT LC07050
Institucionální podpora: RVO:61389005
Klíčová slova: nuclear astrophysics * direct reactions * nucleosynthesis in novae * supernovae * other explosive environments
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
DOI: https://doi.org/10.1063/1.4874068

The role of oxygen in astrophysics is related to different problems as novae nucleosynthesis and gamma-ray astronomy. In particular, owing to the still present uncertainties on its rate, the O-17(p,alpha)N-14 is one of the most important reaction to be studied in order to get more information about the fate of oxygen in different astrophysical scenarios.
Trvalý link: http://hdl.handle.net/11104/0239567