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Thomas G. Bisbas
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Fine-structure lines as diagnostic for cloud-cloud collision activity

  • Post author:Thomas Bisbas
  • Post published:January 6, 2022
  • Post category:Uncategorized
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The dominant process for the galactic star formation is believed to be the collision between giant molecular clouds. The collision triggers the gravitational collapse of the merged clouds, creating star…

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Cosmic-ray induced destruction of CO

  • Post author:Thomas Bisbas
  • Post published:January 6, 2022
  • Post category:Uncategorized
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Ordinary boosts of cosmic-rays (CRs) are able to destroy the molecule of CO very efficiently but not H2, creating vast amounts of the so-called ‘CO-dark’ molecular gas. We have found…

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Determining the ISM environment using probability density functions

  • Post author:Thomas Bisbas
  • Post published:January 6, 2022
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Modern observations of the interstellar medium in galaxies detect a variety of atomic and molecular species. The goal is to connect these observations to the astrochemical properties of the ISM.…

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Development of astrochemical and radiative transfer codes

  • Post author:Thomas Bisbas
  • Post published:January 6, 2022
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I am the main developer of the astrochemical code 3D-PDR. This is an open-source OpenMP-parallelized 3D code. It is specifically designed to treat Photodissociation Regions (PDRs) of arbitrary density distributions.…

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Most recent papers

The impact of cosmic-ray attenuation on the carbon cycle emission in molecular clouds

Photodissociation Region Diagnostics Across Galactic Environments

Contact:

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