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papers

Publications (24)

astro-ph.GA2014

A UV flux constraint on the formation of direct collapse black holes

M. A. Latif, S. Bovino, C. Van Borm +3

astro-ph.GA2016

A detailed framework to incorporate dust in hydrodynamical simulations

T. Grassi, S. Bovino, T. Haugboelle +1

astro-ph.GA2016

Modeling the role of electron attachment rates on column density ratios for CnH-/CnH (n=4,6,8) in dense molecular clouds

F. A. Gianturco, T. Grassi, R. Wester

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

astro-ph.GA2012

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

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

astro-ph.GA2011

ROBO: a Model and a Code for the Study of the Interstellar Medium

T. Grassi, P. Krstic, E. Merlin +3

astro-ph.SR2014

Formation of carbon-enhanced metal-poor stars in the presence of far ultraviolet radiation

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

astro-ph.GA2011

Formation and Evolution of the Dust in Galaxies. III. The Disk of the Milky Way

L. Piovan, C. Chiosi, E. Merlin +4

astro-ph.CO2013

Primordial star formation: relative impact of H2 three-body rates and initial conditions

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

astro-ph.GA2014

Effects of turbulence and rotation on protostar formation as a precursor to seed black holes

C. Van Borm, S. Bovino, M. A. Latif +3

astro-ph.GA2014

Dark-matter halo mergers as a fertile environment for low-mass Population III star formation

S. Bovino, M. A. Latif, T. Grassi +1

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

astro-ph.GA2011

Formation and Evolution of the Dust in Galaxies. I. The Condensation Efficiencies

L. Piovan, C. Chiosi, E. Merlin +4

astro-ph.GA2016

The formation of the primitive star SDSS J102915+172927: effect of the dust mass and the grain-size distribution

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

astro-ph.GA2019

The challenges of modelling microphysics: ambipolar diffusion, chemistry, and cosmic rays in MHD shocks

T. Grassi, M. Padovani, J. P. Ramsey +4

astro-ph.IM2013

Chemical complexity in astrophysical simulations: optimization and reduction techniques

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

astro-ph.GA2014

KROME - a package to embed chemistry in astrophysical simulations

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

astro-ph.CO2013

Impact of an accurate modeling of primordial chemistry in high resolution studies

S. Bovino, T. Grassi, M. A. Latif +1

astro-ph.GA2014

How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes

M. A. Latif, S. Bovino, T. Grassi +2

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

astro-ph.IM2011

MaNN: Multiple Artificial Neural Networks for modelling the Interstellar Medium

T. Grassi, E. Merlin, L. Piovan +2

astro-ph.IM2012

Complexity reduction of astrochemical networks

T. Grassi, S. Bovino, F. A. Gianturco +2

astro-ph.GA2014

The formation of massive primordial stars in the presence of moderate UV backgrounds

M. A. Latif, D. R. G. Schleicher, S. Bovino +2

astro-ph.GA2011

Formation and Evolution of the Dust in Galaxies. II. The Solar Neighbourhood

L. Piovan, C. Chiosi, E. Merlin +4