collaborators

6 papers

astro-ph.GA2025

Turbulence inference from CO spectral observations

Jayashree Narayan, Aris Tritsis, Christoph Federrath

Turbulence influences the structure and dynamics of molecular clouds, and plays a key role in regulating star formation. We therefore need methods to accurately infer turbulence pr…

astro-ph.GA2025

Investigating the role of magnetic fields in the formation and evolution of striations in interstellar clouds with PRIMA

Raphael Skalidis, Konstantinos Tassis, Aris Tritsis +1

Striations are diffuse, linear, quasi-periodic, and magnetized structures located in the outskirts of molecular clouds. These structures seem to play an important role during the e…

astro-ph.GA2025

Ambipolar diffusion and the mass-to-flux ratio in a turbulent collapsing cloud

Aris Tritsis

The formation of stars is governed by the intricate interplay of nonideal magnetohydrodynamic (MHD) effects, gravity, and turbulence. Computational challenges have hindered a compr…

astro-ph.GA2025

A three-step approach to reliably estimate magnetic field strengths in star-forming regions

Aristeidis Polychronakis, Aris Tritsis, Raphael Skalidis +1

The magnetic field is known to play a crucial role in star formation. Dust polarization is an effective tool for probing the morphology of the field, yet it does not directly trace…

astro-ph.GA2025

Projection-angle effects when "observing" a turbulent magnetized collapsing molecular cloud. II. Magnetic field

A. Tritsis, S. Basu, C. Federrath

Interstellar magnetic fields are thought to play a fundamental role in the evolution of star-forming regions. Polarized thermal dust emission serves as a key probe for understandin…

astro-ph.GA2025

A fast and robust recipe for modeling non-ideal MHD effects in star-formation simulations

E. Agianoglou, A. Tritsis, K. Tassis

Non-ideal MHD effects are thought to be a crucial component of the star-formation process. Numerically, several complications render the study of non-ideal MHD effects in 3D simula…