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20032026
most citedThe CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group

572 citations · 4.7k across the 88 of their papers we have counts for

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Showing 2012Show all

6 papers · 1 filter

astro-ph.GA2012★ 23 cited

The hyperfine structure in the rotational spectrum of CF+

V. Guzmán, E. Roueff, J. Gauss +5

Context. CF+ has recently been detected in the Horsehead and Orion Bar photo-dissociation regions. The J=1-0 line in the Horsehead is double-peaked in contrast to other millimeter…

astro-ph.GA2012★ 149 cited

The IRAM-30m line survey of the Horsehead PDR: II. First detection of the l-C3H+ hydrocarbon cation

Jérôme Pety, P. Gratier, V. Guzmán +9

We present the first detection of the l-C3H+ hydrocarbon in the interstellar medium. The Horsehead WHISPER project, a millimeter unbiased line survey at two positions, namely the p…

astro-ph.GA2012★ 7 cited

A detailed view of a Molecular Cloud in the far outer disk of M33

J. Braine, P. Gratier, Y. Contreras +2

The amount of H present in spiral galaxies remains uncertain, particularly in the dim outer regions and in low-metallicity environments. We present high-resolution CO(1--0) obs…

astro-ph.CO2012★ 16 cited

Spectrally resolved CII emission in M~33 ({\tt HerM33es}): Physical conditions and kinematics around BCLMP 691

J. Braine, P. Gratier, C. Kramer +7

This work presents high spectral resolution observations of the \CII\ line at 158 \micron, one of the major cooling lines of the interstellar medium, taken with the HIFI heterodyne…

astro-ph.GA2012★ 49 cited

The IRAM-30m line survey of the Horsehead PDR: I. CF+ as a tracer of C+ and a measure of the Fluorine abundance

V. Guzmán, J. Pety, P. Gratier +4

C+ is a key species in the interstellar medium but its 158 μm fine structure line cannot be observed from ground-based telescopes. Current models of fluorine chemistry predict that…

astro-ph.CO2012★ 73 cited

Dust and gas power-spectrum in M33 (HERM33ES)

F. Combes, M. Boquien, C. Kramer +18

Power spectra of de-projected images of late-type galaxies in gas and/or dust emission are very useful diagnostics of the dynamics and stability of their interstellar medium. Previ…