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19932022
most citedGas-to-Dust mass ratios in local galaxies over a 2 dex metallicity range

661 citations · 8.2k across the 114 of their papers we have counts for

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Showing 2014Show all

15 papers · 1 filter

astro-ph.GA2014★ 12 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.GA2014★ 30 cited

Spatially resolved physical conditions of molecular gas and potential star formation tracers in M83, revealed by the Herschel SPIRE FTS

Ronin Wu, Suzanne Madden, Frédéric Galliano +19

Since the launch of the Herschel Space Observatory, our understanding about the photo-dissociation regions (PDR) has taken a step forward. In the bandwidth of the Fourier Transform…

astro-ph.GA2014★ 44 cited

Far-infrared line spectra of Seyfert galaxies from the Herschel-PACS Spectrometer

Luigi Spinoglio, Miguel Pereira-Santaella, Kalliopi M. Dasyra +4

We present spectroscopic observations of FIR fine-structure lines of 26 Seyfert galaxies obtained with the Herschel-PACS spectrometer. These observations are complemented by spectr…

astro-ph.GA2014★ 41 cited

Insights into gas heating and cooling in the disc of NGC 891 from Herschel far-infrared spectroscopy

T. M. Hughes, K. Foyle, M. R. P. Schirm +15

We present Herschel PACS and SPIRE spectroscopy of the most important far-infrared cooling lines in the nearby edge-on spiral galaxy, NGC 891: [CII] 158 m, [NII] 122, 205 m,…

astro-ph.GA2014★ 16 cited

Quantifying the Heating Sources for Mid-infrared Dust Emissions in Galaxies: The Case of M 81

Nanyao Lu, G. J. Bendo, A. Boselli +12

With the newly available SPIRE images at 250 and 500 micron from Herschel Space Observatory, we study quantitative correlations over a sub-kpc scale among three distinct emission c…

astro-ph.GA2014★ 99 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…