most citedHigh-resolution, 3D radiative transfer modeling : I. The grand-design spiral galaxy M51

99 citations · 176 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2016

FIR extended emission from cold gas and dust in Blue Compact Dwarf Galaxies: the anomalous cases of POX 186 and UM 461

Vanessa Doublier, Aurelie Remy-Ruyer

FIR observation of BCD galaxies with Herschel has revealed a wealth of new insights in these objects which are thought to resemble high-redshift forming galaxies. Dust and cold gas…

astro-ph.GA201631 cited

Far-reaching Dust Distribution in Galaxy Disks

Matthew W. L. Smith, Stephen A. Eales, Ilse De Looze +21

In most studies of dust in galaxies, dust is only detected from its emission to approximately the optical radius of the galaxy. By combining the signal of 110 spiral galaxies obser…

astro-ph.GA201412 cited

The relationship between polycyclic aromatic hydrocarbon emission and far-infrared dust emission from NGC 2403 and M83

A. G. Jones, G. J. Bendo, M. Baes +13

We examine the relation between polycyclic aromatic hydrocarbon (PAH) emission at 8 microns and far-infrared emission from hot dust grains at 24 microns and from large dust grains…

astro-ph.GA201427 cited

The Herschel Virgo Cluster Survey. XVIII. Star-forming dwarf galaxies in a cluster environment

M. Grossi, L. K. Hunt, S. C. Madden +22

To assess the effects of the cluster environment on the different components of the interstellar medium, we analyse the FIR-submm properties of a sample of star-forming dwarf (SFD)…

astro-ph.GA201499 cited

High-resolution, 3D radiative transfer modeling : I. The grand-design spiral galaxy M51

Ilse De Looze, Jacopo Fritz, Maarten Baes +20

Context: Dust reprocesses about half of the stellar radiation in galaxies. The thermal re-emission by dust of absorbed energy is considered driven merely by young stars and, conseq…

astro-ph.GA20147 cited

Probing the interstellar medium of NGC1569 with Herschel

Sophia Lianou, Pauline Barmby, Aurelie Remy-Ruyer +3

NGC1569 has some of the most vigorous star formation among nearby galaxies. It hosts two super star clusters (SSCs) and has a higher star formation rate (SFR) per unit area than ot…