activity
20092026
most citedEvolution of PAHs in photodissociation regions: Hydrogenation and charge states

183 citations · 1.2k across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.IM2026

CosmicPAH-IRDB: A Web Application for Including Anharmonicity in Simulated PAH Spectra for Astrophysics

Louan de Bentzmann, Christine Joblin, Karine Demyk +6

Advances in infrared observations with the James Webb Space Telescope (JWST) call for new tools to exploit the information associated with the Aromatic Infrared Bands (AIBs), now o…

astro-ph.GA2026

Infrared spectroscopy of gas-phase hydrogenated and methylated pyrenes: from laboratory spectra to the simulated 3.4 m emission band

Karine Demyk, Christine Joblin, Louan de Bentzmann +2

Observations of the aromatic infrared emission band at 3.3 mic often reveal satellite emission features in the 3.4 - 3.6 mic range. While the 3.3 mic band is attributed to the CH s…

astro-ph.GA2026

Acenaphthene Derivatives as Signatures of CH Reactivity with Methylated Naphthalenes

Ana I. Lozano, Anthony Bonnamy, Aude Simon +1

CH ion is the dominant fragment cation formed from methyl-naphthalene (MeNp) and dimethyl-naphthalene (diMeNp). Using the multiplex capabilities of PIRENEA, a setup de…

astro-ph.GA2025★ 3 cited

Long-Lived Isomers of CH: New Experimental Insights from the PIRENEA Setup

Ana Isabel Lozano, Anthony Bonnamy, Aude Simon +1

The dehydrogenated cation of methylated benzene is known to exist in two isomeric forms: benzylium and tropylium. Structurally similar forms have been proposed for the -H cations o…

astro-ph.SR2015★ 28 cited

Polycyclic aromatic hydrocarbons and molecular hydrogen in oxygen-rich planetary nebulae: the case of NGC6720

N. L. J. Cox, P. Pilleri, O. Berne +2

Evolved stars are primary sources for the formation of polycyclic aromatic hydrocarbons (PAHs) and dust grains. Their circumstellar chemistry is usually designated as either oxygen…

astro-ph.GA2014★ 132 cited

The chemistry and spatial distribution of small hydrocarbons in UV-irradiated molecular clouds: the Orion Bar PDR

S. Cuadrado, J. R. Goicoechea, P. Pilleri +3

We study the spatial distribution and chemistry of small hydrocarbons in the Orion Bar PDR. We used the IRAM-30m telescope to carry out a millimetre line survey towards the Orion B…

astro-ph.GA2014★ 26 cited

Physical structure of the photodissociation regions in NGC 7023. Observations of gas and dust emission with Herschel

M. Köhler, E. Habart, H. Arab +16

The determination of the physical conditions in molecular clouds is a key step towards our understanding of their formation and evolution of associated star formation. We investiga…

astro-ph.GA2013★ 25 cited

Kinematics of the ionized-to-neutral interfaces in Monoceros R2

P. Pilleri, A. Fuente, M. Gerin +10

Context. Monoceros R2 (Mon R2), at a distance of 830 pc, is the only ultra-compact H ii region (UC H ii) where its associated photon-dominated region (PDR) can be resolved with the…

astro-ph.GA2013★ 1 cited

Detection of the buckminsterfullerene cation (C60+) in space

Olivier Berné, Giacomo Mulas, Christine Joblin

In the early 90s, C60+ was proposed as the carrier of two diffuse interstellar bands (DIBs) at 957.7 and 963.2 nm, but a firm identification still awaits gas-phase spectroscopic da…

astro-ph.GA2013★ 183 cited

Evolution of PAHs in photodissociation regions: Hydrogenation and charge states

J. Montillaud, C. Joblin, D. Toublanc

Various studies have emphasized variations of the charge state and composition of the interstellar polycyclic aromatic hydrocarbon (PAH) population in photodissociation regions (PD…

astro-ph.GA2012★ 42 cited

The chemistry of C3 & Carbon Chain Molecules in DR21(OH)

B. Mookerjea, G. Hassel, M. Gerin +14

(Abridged) We have observed velocity resolved spectra of four ro-vibrational far-infrared transitions of C3 between the vibrational ground state and the low-energy nu2 bending mode…

astro-ph.GA2012★ 142 cited

Evaporating Very Small Grains as tracers of the UV radiation field in Photo-dissociation Regions

P. Pilleri, J. Montillaud, O. Berné +1

Context. In photo-dissociation regions (PDRs), Polycyclic Aromatic Hydrocarbons (PAHs) could be produced by evaporation of Very Small Grains (VSGs) by the impinging UV radiation fi…

astro-ph.GA2011★ 70 cited

OH emission from warm and dense gas in the Orion Bar PDR

J. R. Goicoechea, C. Joblin, A. Contursi +7

As part of a far-infrared (FIR) spectral scan with Herschel/PACS, we present the first detection of the hydroxyl radical (OH) towards the Orion Bar photodissociation region (PDR).…

astro-ph.GA2010★ 35 cited

Gas morphology and energetics at the surface of PDRs: new insights with Herschel observations of NGC 7023

C. Joblin, P. Pilleri, J. Montillaud +37

We investigate the physics and chemistry of the gas and dust in dense photon-dominated regions (PDRs), along with their dependence on the illuminating UV field. Using Herschel-HIFI…

astro-ph.GA2010★ 29 cited

Reversal of infall in SgrB2(M) revealed by Herschel/HIFI observations of HCN lines at THz frequencies

Rainer Rolffs, Peter Schilke, Claudia Comito +54

To investigate the accretion and feedback processes in massive star formation, we analyze the shapes of emission lines from hot molecular cores, whose asymmetries trace infall and…

astro-ph.GA2010★ 20 cited

The origin of the [C II] emission in the S140 PDRs - new insights from HIFI

C. Dedes, M. Röllig, B. Mookerjea +38

Using Herschel's HIFI instrument we have observed [C II] along a cut through S140 and high-J transitions of CO and HCO+ at two positions on the cut, corresponding to the externally…

astro-ph.SR2010★ 31 cited

Herschel observations of EXtra-Ordinary Sources: The Terahertz spectrum of Orion KL seen at high spectral resolution

N. R. Crockett, E. A. Bergin, S. Wang +60

We present the first high spectral resolution observations of Orion KL in the frequency ranges 1573.4 - 1702.8 GHz (band 6b) and 1788.4 - 1906.8 GHz (band 7b) obtained using the HI…

astro-ph.GA2010★ 140 cited

Herschel observations of EXtra-Ordinary Sources: the present and future of spectral surveys with Herschel/HIFI

E. A. Bergin, T. G. Phillips, C. Comito +56

We present initial results from the Herschel GT key program: Herschel observations of EXtra-Ordinary Sources (HEXOS) and outline the promise and potential of spectral surveys with…

astro-ph.GA2010★ 36 cited

Herschel observations of extra-ordinary sources: Detecting spiral arm clouds by CH absorption lines

S. -L. Qin, P. Schilke, C. Comito +67

We have observed CH absorption lines () against the continuum source Sgr~B2(M) using the \textit{Herschel}/HIFI instrument. With the high spectral…

astro-ph.GA2010★ 57 cited

Herschel/HIFI measurements of the ortho/para ratio in water towards Sagittarius B2(M) and W31C

D. C. Lis, T. G. Phillips, P. F. Goldsmith +74

We present Herschel/HIFI observations of the fundamental rotational transitions of ortho- and para-HO and HO in absorption towards Sagittarius~B2(M) and W31C. The…

astro-ph.GA2010★ 101 cited

Herschel/HIFI discovery of interstellar chloronium (HCl)

D. C. Lis, J. C. Pearson, D. A. Neufeld +102

We report the first detection of chloronium, HCl, in the interstellar medium, using the HIFI instrument aboard the \emph{Herschel} Space Observatory. The li…

astro-ph.GA2010★ 51 cited

Strong CH+ J=1-0 emission and absorption in DR21

E. Falgarone, V. Ossenkopf, M. Gerin +30

We report the first detection of the ground-state rotational transition of the methylidyne cation CH+ towards the massive star-forming region DR21 with the HIFI instrument onboard…

astro-ph.GA2010★ 24 cited

HIFI observations of warm gas in DR21: Shock versus radiative heating

V. Ossenkopf, M. Röllig, R. Simon +35

The molecular gas in the DR21 massive star formation region is known to be affected by the strong UV field from the central star cluster and by a fast outflow creating a bright sho…

physics.chem-ph2010★ 56 cited

Visible photodissociation spectroscopy of PAH cations and derivatives in the PIRENEA experiment

F. Useli-Bacchitta, A. Bonnamy, G. Mulas +3

The electronic spectra of gas-phase cationic polycyclic aromatic hydrocarbons (PAHs), trapped in the Fourier Transform Ion Cyclotron Resonance cell of the PIRENEA experiment, have…