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 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)
- Neutral hydrogen in the Shapley supercluster core ─ I. Environmental effects on gas content and galaxy evolution, Monthly Notices of the Royal Astronomical Society, 2026
- Spatially resolved interstellar dust properties in the face-on spiral galaxy M 99 as observed by NIKA2, Astronomy and Astrophysics, 2026
- High-resolution mapping of molecular tori with ALMA, Astronomy and Astrophysics, 2026
- Metal-THINGS: Gas metallicity gradients in nearby galaxies, Astronomy and Astrophysics, 2025
- The role of young and evolved stars in the heating of dust in local galaxies, Astronomy and Astrophysics, 2025
- Radial variation of the silicate-to-carbon ratio in M31 probed by PRIMA, Journal of Astronomical Telescopes, Instruments, and Systems, 2025
- Recovering the dust mass budget with PRIMA, Journal of Astronomical Telescopes, Instruments, and Systems, 2025
- PRIMA survey of the Virgo cluster, Journal of Astronomical Telescopes, Instruments, and Systems, 2025
- Decoding the molecular torus of NGC 1068: Insights into its structure and kinematics from high-resolution ALMA observations, Astronomy and Astrophysics, 2025
- PRIMA promise of deciphering interstellar dust evolution with observations of the nearby Universe, Journal of Astronomical Telescopes, Instruments, and Systems, 2025