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Chemical fingerprints of star forming regions and active galaxies

08 October 2010

PhD ceremony: Mr. J.P. Pérez Beaupuits, 14.45 uur, Academiegebouw, Broerstraat 5, Groningen

Thesis: Chemical fingerprints of star forming regions and active galaxies

Promotor(s): prof. M.C. Spaans

Faculty: Mathematics and Natural Sciences

 

The thesis is devoted to the study of the physical conditions of the interstellar medium (ISM) in active galactic nuclei (AGNs) and Galactic starforming regions, using mostly single-dish millimeter observations. I first study the excitation conditions of dense gas in a group of Seyfert galaxies using radiative transfer models (Chapter 2). I then study the galaxy NGC 1068, and try to distinguish signatures of the contributions from the AGN and the starburst ring by incorporating observations of high-J transitions of dense gas tracers (Chapter 3). Later, I venture into the mid-infrared spectral region to study different aspects of the AGN and starburst components in the galaxy NGC 4945 (Chapter 4). In Chapter 5 I delve into theoretical aspects of the dynamical evolution of gas in an AGN torus. I use a 3D hydrodynamic simulation with chemical abundances driven by X-rays. The aim is to understand the effects of X-ray irradiation by the AGN on the temperature, formation and destruction of the molecular gas. I finally explore a Galactic star-forming region, the Omega Nebula, with high resolution single dish observations, to study the properties of the warm gas and to constrain chemical models (Chapters 6 and 7).

 

Last modified:13 March 2020 01.15 a.m.
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