234 citations · 1.8k across the 57 of their papers we have counts for
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Physical conditions in the gas phases of the giant HII region LMC-N11: II. Origin of [CII] and fraction of CO-dark gas
V. Lebouteiller, D. Cormier, S. C. Madden +11
(abridged) The ambiguous origin of [CII] 158um in the interstellar medium complicates its use for diagnostics concerning the star-formation rate and physical conditions in photodis…
Fingerprinting the effects of hyperfine structure on CH and OH far infrared spectra using Wiener filter deconvolution
Arshia M. Jacob, Karl M. Menten, Helmut Wiesemeyer +3
In this paper, we investigate the influence of hyperfine splitting on complex spectral lines, with the aim of evaluating canonical abundances by decomposing their dependence on hyp…
Herschel spectroscopy of Massive Young Stellar Objects in the Magellanic Clouds
J. M. Oliveira, J. Th. van Loon, M. Sewilo +11
We present Herschel Space Observatory Photodetector Array Camera and Spectrometer (PACS) and Spectral and Photometric Imaging Receiver Fourier Transform Spectrometer (SPIRE FTS) sp…
Exploring the properties of warm and cold atomic hydrogen in the Taurus and Gemini regions
Hiep Nguyen, J. R. Dawson, Min-Young Lee +5
We report Arecibo 21 cm absorption-emission observations to characterise the physical properties of neutral hydrogen (HI) in the proximity of five giant molecular clouds (GMCs): Ta…
Radiative and mechanical feedback into the molecular gas in the Large Magellanic Cloud. II. 30 Doradus
Min-Young Lee, Suzanne Madden, Franck Le Petit +6
With an aim of probing the physical conditions and excitation mechanisms of warm molecular gas in individual star-forming regions, we performed Herschel SPIRE FTS observations of 3…
Observational study of hydrocarbons in the bright photodissociation region of Messier 8
M. Tiwari, K. M. Menten, F. Wyrowski +3
Hydrocarbons are ubiquitous in the interstellar medium, but their formation is still not well understood, depending on the physical environment they are found in. M8 is host to one…