activity
20092013
most citedKROME - a package to embed chemistry in astrophysical simulations

248 citations · 248 across the 1 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2013★ 248 cited

KROME - a package to embed chemistry in astrophysical simulations

T. Grassi, S. Bovino, D. R. G. Schleicher +4

Chemistry plays a key role in many astrophysical situations regulating the cooling and the thermal properties of the gas, which are relevant during gravitational collapse, the evol…

astro-ph.GA2013

CH+ depletion by atomic hydrogen: accuracy of new rates in photo-dominated and self-shielded environments

S. Bovino, T. Grassi, M. Tacconi +1

A detailed quantum analysis of a ionic reaction with a crucial role in the ISM is carried out to generate ab initio reactive cross sections with a quantum method. From them we obta…

astro-ph.GA2012

Carbon Cations and Silicon Atoms in the ISM: modeling their charge exchange reaction

M. Satta, T. Grassi, F. A. Gianturco

The time-dependent rate coefficients for the charge exchange reaction C+ + Si -> C + Si+ for doublet and quartet states have been determined with ab initio quantum calculations cou…

astro-ph.IM2012

Chemical complexity in astrophysical simulations: optimization and reduction techniques

T. Grassi, S. Bovino, D. Schleicher +1

Chemistry has a key role in the evolution of the interstellar medium (ISM), so it is highly desirable to follow its evolution in numerical simulations. However, it may easily domin…

astro-ph.GA2012

Electron attachment rates for PAH anions in the ISM and dark molecular clouds: dependence on their chemical properties

F. Carelli, T. Grassi, F. A. Gianturco

CONTEXT: The attachment of free electrons to polycondensed aromatic ring molecules (PAHs) is studied for the variety of these molecules with different numbers of condensed rings an…

astro-ph.GA2012

Electron-attachment rates for carbon-rich molecules in protoplanetary atmospheres: the role of chemical differences

F. Carelli, T. Grassi, F. Sebastianelli +1

The formation of anionic species in the interstellar medium from interaction of linear molecules containing carbon, nitrogen and hydrogen as atomic components (polyynes) with free…