Items where Author is "Hirschi, R."

Article

den Hartogh, Jacqueline and Hirschi, R. and Lugaro, Maria and Doherty, Carolyn and Battino, U. and Pignatari, Marco (2019) The s process in rotating low-mass AGB stars. Nucleosynthesis calculations in models matching asteroseismic constraints. ASTRONOMY & ASTROPHYSICS, 629. ISSN 0004-6361

Cescutti, G. and Hirschi, R. and Nishimura, N. and Rauscher, T. and den Hartogh, Jacqueline and Murphy, A. St. J. and Cristallo, S. (2019) The s-process nucleosynthesis in low mass stars: impact of the uncertainties in the nuclear physics determined by Monte Carlo variations. SPRINGER PROCEEDINGS IN PHYSICS, 219. pp. 297-300. ISSN 0930-8989

Cescutti, G. and Hirschi, R. and Nishimura, N. and den Hartogh, Jacqueline and Rauscher, T. (2018) Uncertainties in s-process nucleosynthesis in low-mass stars determined from Monte Carlo variations. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 478 (3). pp. 4101-4127. ISSN 0035-8711

Pignatari, Marco and Herwig, F. and Hirschi, R. and Bennett, M. and Rockefeller, G. (2016) NuGrid stellar data set I. Stellar yields from H to Bi for stars with metallicities Z=0.02 and Z= 0.01. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 225 (2). ISSN 0067-0049

Frischknecht, U. and Hirschi, R. and Pignatari, Marco and Maeder, A. and Meynet, G. (2016) s-process production in rotating massive stars at solar and low metallicities. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 456 (2). pp. 1803-1825. ISSN 0035-8711

Barbuy, B. and Chiappini, C. and Cantelli, E. and Depagne, E. and Pignatari, Marco and Hirschi, R. and Cescutti, G. and Ortolani, S. and Hill, V. and Zoccali, M. and Minniti, D. and Trevisan, M. and Bica, E. and Gómez, A. (2014) High-resolution abundance analysis of red giants in the globular cluster NGC 6522. ASTRONOMY & ASTROPHYSICS, 570. ISSN 0004-6361

Pignatari, Marco and Zinner, E. and Bertolli, M. G. and Trappitsch, R. and Hoppe, P. and Rauscher, T. and Fryer, C. and Herwig, F. and Hirschi, R. and Timmes, F. X. and Thielemann, F. -K (2013) Silicon carbide grains of type C provide evidence for the production of the unstable isotope 32Si in supernovae. ASTROPHYSICAL JOURNAL, 771 (1). ISSN 1538-4357