Viviana Casasola

Posizione: Ricercatore

Contatti

  • Stanza: C-612A
  • Telefono: +39 051 6399426
  • Email: casasola@ira.inaf.it

Informazioni personali

Attività

My scientific interests cover the interstellar medium and star formation processes in galaxies, as well as the gas fueling and outflows of active galactic nuclei, with a particular focus on galaxies in the local Universe. I also explore (proto-)clusters of galaxies in the distant Universe. To tackle these topics, I adopt a multi-wavelength approach—from UV to radio—leveraging observations from both ground-based and space telescopes, including ALMA, GALEX, Herschel, HST, JWST, IRAM, JVLA, LBT, MeerKAT, SDSS, and WISE.

Paper più recenti su ADS
(based on ORCID, see here how to claim missing papers)

  1. The role of young and evolved stars in the heating of dust in local galaxies, Astronomy and Astrophysics, 2025
  2. Decoding the molecular torus of NGC 1068: Insights into its structure and kinematics from high-resolution ALMA observations, Astronomy and Astrophysics, 2025
  3. CH3OH as a user-friendly density probe: Calibration and beyond, Astronomy and Astrophysics, 2025
  4. JWST MIRI and NIRCam observations of NGC 891 and its circumgalactic medium, Astronomy and Astrophysics, 2024
  5. Ram-pressure stripped radio tails detected in the dynamically active environment of the Shapley Supercluster, Monthly Notices of the Royal Astronomical Society, 2024
  6. The impact of stellar bars on star-formation quenching: Insights from a spatially resolved analysis in the local Universe, EAS2024, European Astronomical Society Annual Meeting, 2024
  7. Correlations between IR Luminosity, Star Formation Rate, and CO Luminosity in the Local Universe, Galaxies, 2024
  8. The impact of stellar bars on star-formation quenching: Insights from a spatially resolved analysis in the local Universe, Astronomy and Astrophysics, 2024
  9. AGN feedback in the Local Universe: Multiphase outflow of the Seyfert galaxy NGC 5506, Astronomy and Astrophysics, 2024
  10. The ALPINE-ALMA [CII] survey: Dust emission effective radius up to 3 kpc in the early Universe, Astronomy and Astrophysics, 2024
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