148 citations · 1.6k across the 31 of their papers we have counts for
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Polycyclic aromatic hydrocarbons and molecular hydrogen in oxygen-rich planetary nebulae: the case of NGC6720
N. L. J. Cox, P. Pilleri, O. Berne +2
Evolved stars are primary sources for the formation of polycyclic aromatic hydrocarbons (PAHs) and dust grains. Their circumstellar chemistry is usually designated as either oxygen…
The infrared signatures of very small grains in the Universe seen by JWST
Paolo Pilleri, Olivier Berné, Christine Joblin
The near- and mid-IR spectrum of many astronomical objects is dominated by emission bands due to UV-excited polycyclic aromatic hydrocarbons (PAH) and evaporating very small grains…
Variations in solar wind fractionation as seen by ACE/SWICS over a solar cycle and the implications for Genesis Mission results
P. Pilleri, D. B. Reisenfeld, T. H. Zurbuchen +5
We use ACE/SWICS elemental composition data to compare the variations in solar wind fractionation as measured by SWICS during the last solar maximum (1999-2001), the solar minimum…
Very Large Telescope observations of Gomez's Hamburger: Insights into a young protoplanet candidate
O. Berne, A. Fuente, E. Pantin +8
Planets are thought to form in the gas and dust disks around young stars. In particular, it has been proposed that giant planets can form through the gravitational instability of m…
Mixed aliphatic and aromatic composition of evaporating very small grains in NGC 7023 revealed by the 3.4/3.3 m ratio
P. Pilleri, C. Joblin, F. Boulanger +1
In photon-dominated regions (PDRs), UV photons from nearby stars lead to the evaporation of very small grains (VSGs) and the production of gas-phase polycyclic aromatic hydrocarbon…
The chemical footprint of the star formation feedback in M 82 on scales of 100 pc
D. Ginard, A. Fuente, S. García-Burillo +7
We present interferometric observations of the CN 1-0 (113.491 GHz), N2H+ 1-0 (93.173 GHz), H(41)a (92.034 GHz), CH3CN (91.987 GHz), CS 3-2 (146.969 GHz), c-C3H2 3-2 (145.089 GHz),…