40 citations · 78 across the 7 of their papers we have counts for
6 papers
A multilevel implementation of the Goldreich-Kylafis effect into the radiative transfer code PyRaTE
Aris Tritsis, Nikolaos D. Kylafis
Among all the available observational techniques for studying magnetic fields in the dense cold phase of the interstellar medium, linear polarization of spectral lines, referred to…
Can we observe the ion-neutral drift velocity in prestellar cores?
Aris Tritsis, Shantanu Basu, Christoph Federrath
Given the low ionization fraction of molecular clouds, ambipolar diffusion is thought to be an integral process in star formation. However, chemical and radiative-transfer effects,…
CO enhancement by magnetohydrodynamic waves; Striations in the Polaris Flare
R. Skalidis, K. Gkimisi, K. Tassis +4
The formation of molecular gas in interstellar clouds is a slow process, but is enhanced by gas compression. Magnetohydrodynamic (MHD) waves create compressed quasiperiodic linear…
Synthetic Polarization Maps of an Outflow Zone from Magnetohydrodynamic Simulations
Gianfranco Bino, Shantanu Basu, Masahiro N Machida +4
The canonical theory of star formation in a magnetized environment predicts the formation of hourglass-shaped magnetic fields during the prestellar collapse phase. In protostellar…
Non-ideal MHD simulations of subcritical prestellar cores with non-equilibrium chemistry
Aris Tritsis, Christoph Federrath, Karen Willacy +1
Non-ideal magnetohydrodynamic (MHD) effects are thought to be gravity's closest ally in overcoming the support of magnetic fields and in forming stars. Here, we modify the publicly…
Striations in molecular clouds: Streamers or MHD waves?
A. Tritsis, K. Tassis
Dust continuum and molecular observations of the low column density parts of molecular clouds have revealed the presence of elongated structures which appear to be well aligned wit…