activity
20032026
most citedEvolution, nucleosynthesis and yields of low mass AGB stars

439 citations · 6.3k across the 124 of their papers we have counts for

collaborators
Showing 2021Show all

10 papers · 1 filter

astro-ph.SR2021

Oxygen and Aluminum-Magnesium Isotopic Systematics of Presolar Nanospinel Grains from CI Chondrite Orgueil

Nan Liu, Nicolas Dauphas, Sergio Cristallo +2

Presolar oxide grains have been previously divided into several groups (Group 1 to 4) based on their isotopic compositions, which can be tied to several stellar sources. Much of av…

astro-ph.SR2021★ 46 cited

Bottom-up dust nucleation theory in oxygen-rich evolved stars I. Aluminium oxide clusters

David Gobrecht, John M. C. Plane, Stefan T. Bromley +3

Aluminum oxide (alumina, AlO) is a promising candidate as a primary dust condensate in the atmospheres of oxygen-rich evolved stars. Therefore, alumina \textit{seed} pa…

astro-ph.SR2021★ 20 cited

New Multielement Isotopic Compositions of Presolar SiC Grains: Implications for Their Stellar Origins

Nan Liu, Jens Barosch, Larry R. Nittler +5

We report NanoSIMS Si and Mg-Al isotopic data (and C, N, and Ti isotopic data when available) for 85 submicron- to micron-sized presolar SiC grains from the CM2 Murchison meteorite…

nucl-ex2021★ 64 cited

Direct measurement of the 13C(α,n)16O cross section into the s-process Gamow peak

G. F. Ciani, L. Csedreki, D. Rapagnani +45

One of the main neutron sources for the astrophysical s-process is the reaction 13C(α,n)16O, taking place in thermally pulsing Asymptotic Giant Branch stars at temperatures around…

astro-ph.SR2021★ 22 cited

Theoretical estimate of the half-life for the radioactive Cs and Cs in astrophysical scenarios

S. Taioli, D. Vescovi, M. Busso +4

We analyze the CsBa and CsBa decays, which are crucial production channels for Ba isotopes in Asympt…

astro-ph.SR2021★ 42 cited

Presolar grain isotopic ratios as constraints to nuclear and stellar parameters of AGB nucleosynthesis

Sara Palmerini, Maurizio Busso, Diego Vescovi +8

Recent models for evolved Low Mass Stars (with ), undergoing the AGB phase assume that magnetic flux-tube buoyancy drives the formation of C reservoirs…