2021

  • Non-ideal MHD simulations of subcritical prestellar cores with non-equilibrium chemistry arxiv
    A. Tritsis, C. Federrath, K. Willacy, K. Tassis (https://doi.org/10.1093/mnras/stab3740)

    • 2019

  • Probing the cold magnetized Universe with SPICA-POL (B-BOP) arxiv
    Ph. André et al. (including A. Tritsis) (PASA, 36, e029)

  • Magnetic field tomography in two clouds towards Ursa Major using HI fibers arxiv
    A. Tritsis, C. Federrath, V. Pavlidou (ApJ, 873, 38)

    • 2018

  • A new method for probing magnetic field strengths from striations in the interstellar medium arxiv
    A. Tritsis, C. Federrath, N. Schneider, K. Tassis (MNRAS, 481, 5275)

  • Magnetic Seismology of Interstellar Gas Clouds: Unveiling a Hidden Dimension arxiv
    A. Tritsis, K. Tassis (Science, 360, 635)

  • Python Radiative Transfer Emission code (PyRaTE): non-LTE spectral lines simulations arxiv
    A. Tritsis, H. W. Yorke, K. Tassis (MNRAS, 478, 2056)

    • 2016

  • Striations in molecular clouds: Streamers or MHD waves? arxiv
    A. Tritsis, K. Tassis (MNRAS, 462, 3602)

  • Chemistry as a diagnostic of prestellar core geometry arxiv
    A. Tritsis, K. Tassis, K. Willacy (MNRAS, 458, 789)

    • 2015

  • Magnetic Field - Gas Density Relation and Observational Implications Revisited arxiv
    A. Tritsis, G. V. Panopoulou, T. Ch. Mouschovias, K. Tassis, V. Pavlidou (MNRAS, 451, 4384)

    • Conference publications

  • The Musca Molecular Cloud: An Interstellar Symphony Publisher
    A. Tritsis (42nd COSPAR Scientific Assembly, E1.18-21-18)

A copy of my PhD thesis in PDF format can be found here


This work was based (in part) on observations made with Herschel. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.