Neven Tomičić 


Image (NGC 602) credit: NASA/Hubble

Welcome

   My name is Neven Tomičić (doc. dr. sc.), currently working as an assistant professor (Croatian: Docent) at the Faculty of Science (Department of Physics; Croatian: Fizički Odsjek, Prirodoslovno-Matematički Fakultet) at the University of Zagreb. I am a lecturer for the courses "Galaxies" and "Modern astrophysical techniques".

   My scientific interest is probing the physics of the interstellar medium (ISM) in nearby galaxies, such as chemical abundances of gas in nearby galaxies, dust & attenuation effects on star-formation prescriptions, properties of the diffuse ionised gas (DIG) and its effects on star-formation across gas-stripped galaxies. Objects of my work are nearby galaxies at various spatial resolutions, from nearby Andromeda and Triangulum galaxy (resolutions of 1-10 pc), tidally interacting and ram-pressure affected galaxy NGC 2276 (~0.5 kpc resolutions), to the GASP sample of 114 galaxies in groups and clusters (kpc scale resolutions).  I am primarily using the optical integral field unit (IFU) spectra and imaging (Hubble space telescope), and combine them with multi-wavelength images, such as the infra-red imaging (WISE, MIPS, Herschel, ...), ultraviolet images (GALEX, UVIT, ...) and sub-mm and radio (IRAM, ALMA, LOFAR, ...). 

My past employment:

Contact:

neven.lacon@gmail.com 

Office 210

University of Zagreb, Faculty of Science, Department of Physics

(Croatian: Sveučijište u Zagrebu, Prirodoslovno-Matematički Fakultet, Fizički odsjek)