Group by: Item Type | No Grouping
Jump to: Article
Number of items: 6.

Article

Adsley, P, Battino, U, Best, A, Caciolli, A, Guglielmetti, A, Imbriani, G, Jayatissa, H, La Cognata, M, Lamia, L, Masha, E, Massimi, C, Palmerini, S, Tattersall, A and Hirschi, R ORCID: https://orcid.org/0000-0001-8764-6522 (2021) Reevaluation of the Ne-23(alpha, gamma)Mg-26 and Ne-22(alpha, n)Mg-25 reaction. PHYSICAL REVIEW C, 103 (1).

Battino, U, Tattersall, A, Lederer-Woods, C, Herwig, F, Denissenkov, P, Hirschi, R, Trappitsch, R, den Hartogh, JW, Pignatari, M and Collaboration, TN (2019) NuGrid stellar data set – III. Updated low-mass AGB models and s-process nucleosynthesis with metallicities Z= 0.01, Z = 0.02, and Z = 0.03. Monthly Notices of the Royal Astronomical Society, 489 (1). 1082 -1098.

den Hartogh, JW, Hirschi, R, Lugaro, M, Doherty, CL, Battino, U, Herwig, F, Pignatari, M and Eggenberger, P (2019) The s process in rotating low-mass AGB stars - Nucleosynthesis calculations in models matching asteroseismic constraints. Astronomy and Astrophysics, 629. A123 -A123.

den Hartogh, J W, Hirschi, R, Georgy, C, Eggenberger, P, Herwig, F, Pignatari, M, Battino, U, Keown, Jared and Ritter, C (2018) Impact of rotation and magnetic fields in low mass AGB stars. Journal of Physics: Conference Series, 940. 012038.

Pignatari, M, Herwig, F, Hirschi, R, Bennett, M, Rockefeller, G, Fryer, C, Timmes, FX, Ritter, C, Heger, A, Jones, S, Battino, U, Dotter, A, Trappitsch, R, Diehl, S, Frischknecht, U, Hungerford, A, Magkotsios, G, Travaglio, C and Young, P (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).

Battino, U, Pignatari, M, Ritter, C, Herwig, F, Denisenkov, P, Den Hartogh, JW, Trappitsch, R, Hirschi, R, Freytag, B, Thielemann, F and Paxton, B (2016) Application of a theory and simulation-based convective boundary mixing model for AGB star evolution and nucleosynthesis. Astrophysical Journal, 827 (1). p. 30.

This list was generated on Wed Nov 1 00:03:48 2023 UTC.