activity
19992026
most citedEvolution, nucleosynthesis and yields of low mass AGB stars

439 citations · 3.1k across the 58 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

physics.ins-det2019

Review and new concepts for neutron-capture measurements of astrophysical interest

C. Domingo-Pardo, V. Babiano-Suarez, J. Balibrea-Correa +128

The idea of slow-neutron capture nucleosynthesis formulated in 1957 triggered a tremendous experimental effort in different laboratories worldwide to measure the relevant nuclear p…

astro-ph.SR2019★ 43 cited

Comprehensive models of novae at metallicity and

Hai-Liang Chen, T. E. Woods, L. R. Yungelson +3

Novae are the observational manifestations of thermonuclear runaways on the surface of accreting white dwarfs (WDs). Although novae are an ubiquitous phenomenon, their properties a…

astro-ph.SR2019★ 25 cited

The initial mass-final luminosity relation of type II supernova progenitors. Hints of new physics?

Oscar Straniero, Inma Dominguez, Luciano Piersanti +2

We revise the theoretical initial mass-final luminosity relation for progenitors of type IIP and IIL supernovae. The effects of the major uncertainties, as those due to the treatme…

astro-ph.SR2019

Thermonuclear oubursts of AM CVn stars

L. R. Yungelson, L. Piersanti, A. Tornambé +1

We consider initial stage of the evolution of AM CVn type stars with white dwarf donors, which is accompanied by thermonuclear explosions in the layer of accreted He. It is shown t…

astro-ph.SR2019★ 19 cited

The effects of a revised Be e-capture rate on solar neutrino fluxes

D. Vescovi, L. Piersanti, S. Cristallo +5

The electron-capture rate on Be is the main production channel for Li in several astrophysical environments. Theoretical evaluations have to account for not only the nuclea…

astro-ph.SR2019★ 9 cited

He-accreting WD: Nucleosynthesis in the extreme binary system (1.02+0.30) M

L. Piersanti, L. R. Yungelson, S. Cristallo +1

We investigate the evolutionary properties of AM~CVn stars with massive white dwarf donors and accretors. As a representative of them we consider a binary initially composed by a 0…