Maria Elisabetta Palumbo

TL;DR: In this paper , the abundance and distribution of ice in PPDs is determined within the uncertainty of the physical parameter space by modeling ice absorption features and determining how well the abundance of the main ice species across the disk can be determined.

TL;DR: In this article , the authors compared the infrared spectra of laboratory-made refractory organic residues to spectra from meteorites and interplanetary dust particles, and confirmed the detection of water, nitriles, hydrocarbons, and carbonates in extraterrestrial particles and link the formation location of the particles in the outer regions of the solar nebula.

TL;DR: In this article, the authors investigated a possible solid phase route of formation for methyl formate (HCOOCH3) in dark clouds, but not that found in hot cores and corinos.

TL;DR: In this article , the authors fit a parameterized dust model to the edge-on protoplanetary disk HH 48 NE by coupling the radiative transfer code RADMC-3D and an MCMC framework.

TL;DR: In this article, an accurate line list of the two HCSSH $trans$ and $cis$ isomers in their electronic ground state and a comprehensive centrifugal distortion analysis with an extension of measurements in the millimetre and submillimetre range were provided.