s-process production in rotating massive stars at solar and low metallicities

By U. Frischknecht, R. Hirschi, M. Pignatari, Andre Maeder, G. Meynet, C. Chiappini, Friedrich-Karl Thielemann, T. Rauscher, C. Georgy, S. Ekström. 2015

157 citations recorded by the source corpus.

This article has been accepted for publication by Monthly Notices of the Royal Astronomical Society. © The Authors. Published by the Oxford University Press on behalf of the Royal Astronomical Society.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/05a565d03db65b13a57a78e0940f1e48c7e0c1f0

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. J. Cowan
2. C. Sneden
3. M. Limongi
4. A. Chieffi
5. J. E. Lawler
6. Friedrich-Karl Thielemann
7. G. Mart'inez-Pinedo
8. N. Prantzos

In Nuclear and High Energy Physics

1. A. Chieffi
2. M. Limongi
3. J. Cowan
4. C. Sneden
5. G. Mart'inez-Pinedo
6. J. E. Lawler
7. K. Langanke
8. Friedrich-Karl Thielemann

Citations in the corpus

• Origin of the heaviest elements: The rapid neutron-capture process (2019, background): “rates contributed already some s-process in early galactic evolution (Frischknecht et al., 2016), this could be due”
• Chemical evolution with rotating massive star yields - I. The solar neighbourhood and the s-process elements (2018, methodology): “…yields: effects (i) to (iii) were studied with yields mainly from Hirschi (2007), while effect (iv) with yields from Frischnecht (2011, PhD Thesis), Frischknecht et al. (2012) and Frischknecht et al. (2016), where stars of different masses, metallicities and rotational velocities were considered.”