activity
19962023
most citedThe 2014 KIDA network for interstellar chemistry

399 citations · 1.4k across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2023

Survival of fossil fields during the pre-main sequence evolution of intermediate-mass stars

Dominik R. G. Schleicher, Juan Pablo Hidalgo, Daniele Galli

Chemically peculiar Ap and Bp stars host strong large-scale magnetic fields in the range of ~G up to ~kG, which are often considered to be the origin of fossil magnetic fi…

astro-ph.SR2022★ 5 cited

Non-ideal magnetohydrodynamics of self-gravitating filaments

Nicol Gutiérrez-Vera, Tommaso Grassi, Stefano Bovino +3

Filaments have been studied in detail through observations and simulations. A range of numerical works have separately investigated how chemistry and diffusion effects, as well as…

astro-ph.GA2015★ 399 cited

The 2014 KIDA network for interstellar chemistry

V. Wakelam, J. -C. Loison, E. Herbst +21

Chemical models used to study the chemical composition of the gas and the ices in the interstellar medium are based on a network of chemical reactions and associated rate coefficie…

astro-ph.SR2009★ 123 cited

Enhanced production of barium in low-mass stars: evidence from open clusters

Valentina D'Orazi, Laura Magrini, Sofia Randich +3

We report the discovery of a trend of increasing barium abundance with decreasing age for a large sample of Galactic open clusters. The observed pattern of [Ba/Fe] vs. age can be r…

astro-ph2006★ 155 cited

Gravitational collapse of magnetized clouds. I. Ideal MHD accretion flow

D. Galli, S. Lizano, F. H. Shu +1

We study the self-similar collapse of an isothermal magnetized rotating cloud in the ideal magnetohydrodynamic (MHD) regime. In the limit of small distance from the accreting proto…

astro-ph2002★ 70 cited

Deuterium chemistry in the primordial gas

D. Galli, F. Palla

We review and update some aspects of deuterium chemistry in the post-recombination Universe with particular emphasis on the formation and destruction of HD. We examine in detail th…