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Marcella Brusa

Full Professor

Department of Physics and Astronomy "Augusto Righi"

Academic discipline: PHYS-05/A Astrophysics, Cosmology and Space Science

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Tesi disponibili per la Laurea Magistrale in Astrofisica e Cosmologia

Elenco e descrizione delle tesi disponibili nell'ambito del tema di ricerca della co-evoluzione galassie e AGN.

 

1) The environment of an obscured, outflowing QSO at z~1.5
goal: characterise the dust and SF properties of a bright submm source, its gas content, and assess the physical relation with a bright obscured QSO at ~170 projected kpc
collaborators: R. Paladino (INAF-IRA)


2) The radio emission in a X-ray luminous CSS with strong ionised wind at z~1.5
goal: assess the role of jets and sub-kpc radio emission in driving outflows
collaborator: I. Delvecchio (Zagreb University)

 

3) Lyman-α emission in a sample of z~2-4 galaxies in COSMOS
goal: study of inflows/outflows interplay in ionised gas around Ly alpha emitters and comparison with stellar kinematics and galaxy morphology
collaborator: M. Mignoli (INAF-OABo)

4) Unveiling AGN excitation in 5 X-ray Bright Optically Normal Galaxies (XBONGs)
goal: disentangle host galaxies and AGN light in these peculiar systems, and map the stellar and extended narrow line region kinematics
collaborator: M. Mignoli + A. Comastri (INAF-OABo)

5) X-ray properties of galaxies with HI outflows
goal: assess X-ray properties and/or other phases outflows incidence in radio selected galaxies with HI outflows
collaborator: G. Lanzuisi (DIFA)

6) Mass without radiation: Heavily obscured AGNs, the X-ray background, and the black hole mass density
goal: derive observational constraints to be used to search for the most obscured AGN responsible for the XRB
collaborator: A. Comastri (INAF-OABo)

7) The cold side of AGN: dust, gas, and star formation in high-z AGN from Herschel and ALMA
goal: construct average SED of AGN in luminosity classes, investigate their dust and gas content and compare them to “normal” galaxies
collaborator: R. Decarli (INAF-OABo)

 

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