Dahbia Talbi

most citedThe ortho-to-para ratio of H

_{2}

^{+}

: Quasi-classical trajectory calculations and new simulations in light of new observations

11 citations · 12 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.GA2025★ 1 cited

Revisiting the formation of molecules and dust in core collapse supernovae

Isabelle Cherchneff, Dahbia Talbi, José Cernicharo

Context. Core-collapse Supernovae of Type II contribute the chemical enrichment of galaxies through explosion. Their role as dust producers in the high-redshift Universe may be of…

astro-ph.GA2017★ 11 cited

The ortho-to-para ratio of H $_{2}$ Cl $^{+}$ : Quasi-classical trajectory calculations and new simulations in light of new observations

Romane Le Gal, Changjian Xie, Eric Herbst +3

Multi-hydrogenated species with proper symmetry properties can present different spin configurations, and thus exist under different spin symmetry forms, labeled as para and ortho…

Revisiting the formation of molecules and dust in core collapse supernovae

The ortho-to-para ratio of H2​Cl+: Quasi-classical trajectory calculations and new simulations in light of new observations

The ortho-to-para ratio of H $_{2}$ Cl $^{+}$ : Quasi-classical trajectory calculations and new simulations in light of new observations