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20132020
most citedThe Herschel Dwarf Galaxy Survey: I. Properties of the low-metallicity ISM from PACS spectroscopy

234 citations · 641 across the 13 of their papers we have counts for

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26 papers · 1 filter

astro-ph.GA202026 cited

SOFIA/FIFI-LS Full-disk [CII] Mapping and CO-dark Molecular Gas across the Nearby Spiral Galaxy NGC 6946

F. Bigiel, I. de Looze, A. Krabbe +17

We present SOFIA/FIFI-LS observations of the [CII] 158m cooling line across the nearby spiral galaxy NGC 6946. We combine these with UV, IR, CO, and H I data to compare [CII] em…

astro-ph.GA2020

Tracing the total molecular gas in galaxies: [CII] and the CO-dark gas

S. C. Madden, D. Cormier, S. Hony +11

While the CO(1-0) transition is often used to deduce the total molecular hydrogen in galaxies, it is challenging to detect in low metallicity galaxies, in spite of the star formati…

astro-ph.GA20207 cited

Local starburst conditions and formation of GRB 980425 / SN 1998bw within a collisional ring

M. Arabsalmani, F. Renaud, S. Roychowdhury +9

We present the first spatially resolved study of molecular gas in the vicinity of a Gamma Ray Burst, using CO(2-1) emission line observations with the Atacama Large Millimetre Arra…

astro-ph.GA202044 cited

The CO-dark molecular gas mass in 30 Doradus

Mélanie Chevance, Suzanne C. Madden, Christian Fischer +16

Determining the efficiency with which gas is converted into stars in galaxies requires an accurate determination of the total reservoir of molecular gas mass. However, despite bein…

astro-ph.GA2020

ALMA Observations of the Molecular Clouds in NGC 625

Nia Imara, Ilse De Looze, Christopher M. Faesi +1

We present the highest resolution (1") CO(1-0) observations of molecular gas in the dwarf starburst galaxy NGC 625, to date, obtained with ALMA. Molecular gas is distributed…

astro-ph.GA2020

Deceptively cold dust in the massive starburst galaxy GN20 at

Isabella Cortzen, Georgios E. Magdis, Francesco Valentino +13

We present new observations, carried out with IRAM NOEMA, of the atomic neutral carbon transitions [CI](1-0) at 492 GHz and [CI](2-1) at 809 GHz of GN20, a well-studied star-bursti…