activity
20232026
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7 papers · 1 filter

astro-ph.GA2026

Optical constants of Ih, Ic, and amorphous HO ices in the THz and IR ranges

A. A. Gavdush, F. Ribeiro, M. K. Matveishina +9

Direct measurements of optical constants in the THz spectral region for astrophysically relevant HO ice samples are scarce. Extrapolation of optical properties in the THz spect…

astro-ph.GA2026

Probing the ion-neutral drift velocity towards the L1544 prestellar core: Detection of ambipolar diffusion using ND and para-NHD

Doris Arzoumanian, Silvia Spezzano, Tommaso Grassi +9

The dynamical role of the magnetic field in the star formation process is tightly linked to the coupling between matter and the field. This coupling is due to the interaction betwe…

astro-ph.GA2026

A differentiable and optimizable 3D model for interpretation of observed spectral data cubes

T. Grassi, J. E. Pineda, S. Spezzano +6

Molecular spectral cubes of prestellar cores encode the information on the physical and chemical properties of these objects along the line of sight. To retrieve this information,…

astro-ph.GA20254 cited

Impact of cosmic-ray propagation on the chemistry and ionisation fraction of dark clouds

G. Latrille, A. Lupi, S. Bovino +3

A proper modelling of the cosmic-ray ionisation rate within gas clouds is crucial to describe their chemical evolution accurately. However, this modelling is computationally demand…

astro-ph.GA20256 cited

Mapping Synthetic Observations to Prestellar Core Models: An Interpretable Machine Learning Approach

T. Grassi, M. Padovani, D. Galli +6

Observations of molecular lines are a key tool to determine the main physical properties of prestellar cores. However, not all the information is retained in the observational proc…

astro-ph.GA2024

Testing analytical methods to derive the cosmic-ray ionisation rate in cold regions via synthetic observations

E. Redaelli, S. Bovino, A. Lupi +4

Cosmic rays (CRs) heavily impact the chemistry and physics of cold and dense star-forming regions. However, characterising their ionisation rate is still challenging from an observ…