activity
20162023
most citedRadial distribution of dust, stars, gas, and star-formation rate in DustPedia face-on galaxies

136 citations · 594 across the 20 of their papers we have counts for

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Showing astro-ph.GAShow all

30 papers · 1 filter

astro-ph.GA202312 cited

The stratification of ISM properties in the edge-on galaxy NGC 891 revealed by NIKA2

S. Katsioli, E. M. Xilouris, C. Kramer +60

As the millimeter wavelength range remains a largely unexplored spectral region for galaxies, the IMEGIN large program aims to map the millimeter continuum emission of 22 nearby ga…

astro-ph.GA202255 cited

METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. III. Interstellar Depletions, Dust-to-Metal, and Dust-to-Gas Ratios Versus Metallicity

J. Roman-Duval, E. B. Jenkins, K. Tchernyshyov +9

The metallicity and gas density dependence of interstellar depletions, the dust-to-gas (D/G), and dust-to-metal (D/M) ratios have important implications for how accurately we can t…

astro-ph.GA20217 cited

Probing the spectral shape of dust emission with the DustPedia galaxy sample

Angelos Nersesian, Wouter Dobbels, Manolis E. Xilouris +10

The objective of this paper is to understand the variance of the far-infrared (FIR) spectral energy distribution (SED) of the DustPedia galaxies, and its link with the stellar and…

astro-ph.GA20212 cited

The Quest for the Missing Dust: I -- Restoring Large Scale Emission in Herschel Maps of Local Group Galaxies

Christopher J. R. Clark, Julia C. Roman-Duval, Karl D. Gordon +2

Because the galaxies of the Local Group have such large angular sizes, much of their diffuse, large-angular-scale emission is filtered out by the Herschel data reduction process. I…

astro-ph.GA202143 cited

METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. II. Variations of interstellar depletions and dust-to-gas ratio within the LMC

Julia Roman-Duval, Edward B. Jenkins, Kirill Tchernyshyov +9

A key component of the baryon cycle in galaxies is the depletion of metals from the gas to the dust phase in the neutral ISM. The METAL (Metal Evolution, Transport and Abundance in…

astro-ph.GA2020

High-resolution, 3D radiative transfer modelling V. A detailed model of the M51 interacting pair

Angelos Nersesian, Sebastien Viaene, Ilse De Looze +13

Investigating the dust heating mechanisms in galaxies provides a deeper understanding of how the internal energy balance drives their evolution. Over the last decade, radiative tra…