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20092026
most citedA panchromatic spatially resolved analysis of nearby galaxies -- II. The main sequence - gas relation at sub-kpc scale in grand-design spirals

56 citations · 247 across the 21 of their papers we have counts for

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15 papers · 1 filter

astro-ph.GA2026

The bar-driven central complex of NGC 6946: A panchromatic and spatially resolved view of its star formation history and interstellar medium

Santiago Álvarez-Córdoba, Jacopo Fritz, M. A. Lara-López +14

We present a multi-wavelength analysis of the nearby spiral galaxy NGC 6946, combining optical IFS, infrared, and radio observations. We aim to characterise both the integrated and…

astro-ph.GA2026

From Scaling Relations to Physical Laws: Constraining the Physics of Star Formation Across Local Galaxies

Jakob den Brok, Cecilia Bacchini, Leindert A. Boogaard +21

The conversion of cold dense gas, traced by molecular line emission, into stars remains one of the fundamental unsolved problems in galaxy evolution. Observations over the past dec…

astro-ph.GA2026

Resolved Dust-Gas-Metallicity relations in nearby spiral galaxies

Vidhi Tailor, Viviana Casasola, Francesco Calura +17

Context: Understanding the interstellar medium (ISM) requires high-resolution, multi-component mapping to capture its complex physical structure. Nearby spiral galaxies, with their…

astro-ph.GA2026

Tracing the Cosmic web across Cosmic time through SKA observations of radio galaxies

Pratik Dabhade, Gianluca Castignani, Mousumi Mahato +4

The Square Kilometre Array will transform studies of the cosmic web by tracing radio galaxies (RGs) and star-forming systems across cosmic time with unprecedented sensitivity, angu…

astro-ph.GA2026

Advancing extragalactic spectral line studies with the Square Kilometre Array Observatory

Jacco Th. van Loon, Viviana Casasola, Manuela Bischetti +6

We present an overview of the Square Kilometre Array Observatory (SKAO) science potential in the area of extragalactic spectral lines besides 21-cm neutral hydrogen. It highlights…

astro-ph.GA2025

Recovering the Dust Mass Budget with PRIMA

A. Traina, F. Pozzi, F. Calura +8

Achieving a complete picture of galaxy evolution is a primary goal of extragalactic astrophysics. To accomplish this ambitious task, a wealth of multi-wavelength surveys have been…

astro-ph.GA2024

Ram-pressure stripped radio tails detected in the dynamically active environment of the Shapley Supercluster

P. Merluzzi, T. Venturi, G. Busarello +13

We study the radio continuum emission of four galaxies experiencing ram-pressure stripping in four clusters of the Shapley supercluster at redshift z~0.05. Multi-band (235-1367 MHz…

astro-ph.GA2024

Correlations between IR Luminosity, Star Formation Rate, and CO Luminosity in the Local Universe

Matteo Bonato, Ivano Baronchelli, Viviana Casasola +5

We exploit the DustPedia sample of galaxies within approximately 40 Mpc, selecting 388 sources, to investigate the correlations between IR luminosity (L), the star forma…

astro-ph.GA2024★ 13 cited

The impact of stellar bars on star-formation quenching: Insights from a spatially resolved analysis in the local Universe

Letizia Scaloni, Giulia Rodighiero, Andrea Enia +8

Stellar bars are common morphological structures in the local Universe; according to optical and NIR surveys, they are present in about two-thirds of disc galaxies. These elongated…

astro-ph.GA2024

Ancient stellar populations in the outskirts of nearby grand-design spirals: Investigation of their star formation histories

Cristina Maria Lofaro, Giulia Rodighiero, Andrea Enia +7

The main sequence (MS) of star-forming galaxies (SFGs) is the tight relation between the galaxy stellar mass and its star formation rate (SFR) and was observed up to z ~ 6. The MS…

astro-ph.GA2023

Modelling molecular clouds and CO excitation in AGN-host galaxies

Federico Esposito, Livia Vallini, Francesca Pozzi +9

We present a new physically-motivated model for estimating the molecular line emission in active galaxies. The model takes into account (i) the internal density structure of giant…

astro-ph.GA2023★ 5 cited

A Bayesian chemical evolution model of the DustPedia Galaxy M74

Francesco Calura, Marco Palla, Laura Morselli +8

We introduce a new, multi-zone chemical evolution model of the DustPedia galaxy M74, calibrated by means of MCMC methods. We take into account the observed stellar and gas density…

astro-ph.GA2020★ 56 cited

A panchromatic spatially resolved analysis of nearby galaxies -- II. The main sequence - gas relation at sub-kpc scale in grand-design spirals

Laura Morselli, Giulia Rodighiero, Andrea Enia +13

In the second work of this series, we analyse the connection between the availability of gas and the position of a region with respect to the spatially resolved main sequence (MS)…

astro-ph.GA2019★ 42 cited

The AGN fuelling/feedback cycle in nearby radio galaxies II. Kinematics of the molecular gas

Ilaria Ruffa, Timothy A. Davis, Isabella Prandoni +7

This is the second paper of a series exploring the multi-component (stars, warm and cold gas and radio jets) properties of a sample of eleven nearby low excitation radio galaxies (…

astro-ph.GA2013★ 50 cited

ALMA observations of cool dust in a low-metallicity starburst, SBS0335-052

L. K. Hunt, L. Testi, V. Casasola +9

We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 0 Band 7 observations of an extremely metal-poor dwarf starburst galaxy in the Local Universe, SBS0335-052 (12+…