Viviana Casasola
Posizione: Ricercatore
Contatti
- Stanza: C-612A
- Telefono: +39 051 6399426
- Email: casasola@ira.inaf.it
Informazioni personali
- Orcid: 0000-0002-3879-6038
Attività
My scientific interests span from the characterization of the interstellar medium of galaxies and star formation processes to the study of the gas fueling and outflow of the active galactic nuclei in the galaxy centers, with particular reference to galaxies of the local Universe. I also study galaxy (proto-)clusters of the distant Universe. In order to achieve these goals, I adopt a multi-wavelength (from UV to radio) approach by using observations coming from both ground-based and spatial telescopes such as ALMA, GALEX, Herschel, HST, IRAM, JVLA, LBT, MeerKAT, SDSS and WISE.
Paper più recenti su ADS
(based on ORCID, see here how to claim missing papers)
- Correlations between IR Luminosity, Star Formation Rate, and CO Luminosity in the Local Universe, Galaxies, 2024
- The impact of stellar bars on star-formation quenching: Insights from a spatially resolved analysis in the local Universe, Astronomy and Astrophysics, 2024
- AGN feedback in the Local Universe: Multiphase outflow of the Seyfert galaxy NGC 5506, Astronomy and Astrophysics, 2024
- The ALPINE-ALMA [CII] survey: Dust emission effective radius up to 3 kpc in the early Universe, Astronomy and Astrophysics, 2024
- Ancient stellar populations in the outskirts of nearby grand-design spirals: Investigation of their star formation histories, Astronomy and Astrophysics, 2024
- ALMA Band 3 Source Counts: A Machine Learning Approach to Contamination Mitigation below 5 Sigma, Galaxies, 2024
- Modelling molecular clouds and CO excitation in AGN-host galaxies, Monthly Notices of the Royal Astronomical Society, 2024
- A Bayesian chemical evolution model of the DustPedia galaxy M74, Monthly Notices of the Royal Astronomical Society, 2023
- Gas, dust, and the CO-to-molecular gas conversion factor in low-metallicity starbursts, Astronomy and Astrophysics, 2023
- One-Stop Shopping: Pan-Metallicity PAH Benchmarking in M101, JWST Proposal. Cycle 2, 2023