Abstract
In this contribution we discuss about numerical modeling of nebulae. In particular we emphasize on the dynamical evolution of an H ii region and on the chemical structure of a Photodissociation region. We do this by using the Smoothed Particles Hydrodynamics code SEREN and the recently developed astrochemistry code 3D-PDR. We show an example application by simulating a cometary globule using these two codes.
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Notes
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known also as “Photon Dominated Region”.
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Acknowledgements
TGB acknowledges support by STFC grant ST/H001794/1.
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Bisbas, T.G. (2014). A Nebula in Your Computer: Simulating the Physics and Chemistry of an H ii Region. In: Stamatellos, D., Goodwin, S., Ward-Thompson, D. (eds) The Labyrinth of Star Formation. Astrophysics and Space Science Proceedings, vol 36. Springer, Cham. https://doi.org/10.1007/978-3-319-03041-8_38
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DOI: https://doi.org/10.1007/978-3-319-03041-8_38
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