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Absolute cross-section measurements for valence-shell photoionization of Ar$^{+}$ ions are reported for photon energies ranging from 27.4 eV to 60.0 eV. The data, taken by merging beams of ions and synchrotron radiation at a photon energy…

This paper describes a near-UV/VIS study of a pyrene:H_2O interstellar ice analogue at 10 K using optical absorption spectroscopy. A new experimental approach makes it possible to irradiate the sample with vacuum ultraviolet (VUV) light…

Instrumentation and Methods for Astrophysics · Physics 2009-08-05 J. Bouwman , D. M. Paardekooper , H. M. Cuppen , H. Linnartz , L. J. Allamandola

PIRENEA and PIRENEA 2 are experimental setups dedicated to the study of fundamental molecular processes involving species of astrochemical interest. The coupling of a VUV source to PIRENEA has allowed us to study the fragmentation pathways…

Instrumentation and Methods for Astrophysics · Physics 2022-08-22 A Marciniak , A Bonnamy , S Zamith , L Noguès , O Coeur-Joly , D Murat , P Moretto-Capelle , J. -M l'Hermite , G Mulas , C Joblin

Steric effect in the threshold dissociative ionizations of serine conformers [CH2OH-C\alphaH(NH2)-C\betaOOH] is revealed by high-level ab initio calculations combined with our newly developed infrared laser desorption / tunable VUV…

Chemical Physics · Physics 2008-07-02 Shan Xi Tian , Jinlong Yang , Hai-Bei Li , Yang Pan , Taichang Zhang , Liusi Sheng

Two key questions of the chemistry of Polycyclic Aromatic Hydrocarbons (PAHs) in the interstellar medium (ISM) are addressed: i) the way carbon is returned from PAHs to the interstellar gas after the very efficient accretion of C+ ions onto…

Astrophysics of Galaxies · Physics 2025-05-14 Alain Omont , Holger F. Bettinger

Two measurements of the energy resolution were performed at MAX-Lab in Lund, Sweden, with an array of 3$\times$3 PbWO4 crystals using a tagged photon beam with energies between 19 and 56 MeV. The crystals were cooled down to -15 and -25…

Nuclear Experiment · Physics 2008-05-08 Sophie Grape

Fragmentation is an important decay mechanism for polycyclic aromatic hydrocarbons (PAHs) under harsh interstellar conditions and represents a possible formation pathway for small molecules such as H2, C2H2, C2H4. Our aim is to investigate…

At the Heidelberg Ion-Beam Therapy Center, the track structure of carbon ions of therapeutic energy after penetrating layers of simulated tissue was investigated for the first time. Measurements were conducted with carbon ion beams of…

Medical Physics · Physics 2025-10-20 Gerhard Hilgers , Miriam Schwarze , Hans Rabus

We investigate the emission properties of polycyclic aromatic hydrocarbons (PAHs) in various metallicity environments with the Infrared Spectrograph on board Spitzer. Local giant HII regions are used as references as they enable access to…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 V. Lebouteiller , J. Bernard-Salas , D. G. Whelan , B. Brandl , F. Galliano , V. Charmandaris , S. Madden , D. Kunth

We report on two pion-photoproduction measurements in the threshold region conducted in the A2 collaboration at MAMI with the almost 4{\pi} Crystal Ball detector. The first was with a linearly polarized photon beam and unpolarized…

Nuclear Experiment · Physics 2013-08-13 David Hornidge

An ongoing discussion revolves around the question of what effect hydrogenation has on carbon backbone fragmentation in Polycyclic Aromatic Hydrocarbons (PAHs). In order to shed more light on this issue, we have measured absolute single…

The electron-detachment energy is measured by its ionization potential (IP). As a result, it is a fundamental observable and important molecular electronic signature in photoelectron spectroscopy. A precise theoretical prediction of…

Chemical Physics · Physics 2023-07-26 Saddem Mamache , Marta Gałyńska , Katharina Boguslawski

We report on the absorption spectra of the polycyclic aromatic hydrocarbon (PAH) molecules anthracene, phenanthrene, and pyrene carrying either an ethynyl (-C2H) or a butadiynyl (-C4H) group. Measurements were carried out in the mid…

Ionization of gas-phase organic molecules such as polycyclic aromatic hydrocarbons (PAHs) requires vacuum ultraviolet photons at wavelengths shorter than 200 nm (~6-9 eV). We present here for the first time that visible photons - accessible…

Astrophysics of Galaxies · Physics 2021-07-07 Antti Lignell , Laura I. Tanalenda-Ossorio , Murthy S. Gudipati

The aromatic infrared Bands (AIBs) dominate the mid-infrared spectra of many galactic and extragalactic sources. These AIBs are generally attributed to fluorescent emission from aromatic molecules. Unified efforts from experimentalists and…

Astrophysics of Galaxies · Physics 2024-08-26 P. Sundararajan , A. Candian , J. Kamer , H. Linnartz , A. G. G. M. Tielens

Methylated polycyclic aromatic hydrocarbons (PAHs) have been hypothesised to be present in the interstellar medium (ISM) through their 3.4 and 6.9 $\mu$m absorption bands. To investigate the hydrogenation of these methylated PAHs, the…

Astrophysics of Galaxies · Physics 2026-02-11 A. T. Hopkinson , F. G. Doktor , J. Pitfield , M. Moll , J. D. Thrower , L. Hornekær

The ionization dynamics of a Xenon cluster with 40 atoms is analyzed under a pum p probe scenario of laser pulses where an infrared laser pulse of 50 fs length follows with a well defined time delay a VUV pulse of the same length and peak…

Atomic and Molecular Clusters · Physics 2009-11-10 Ch. Siedschlag , J. M. Rost

We suggest an explanation of the recently observed discrepancy between the experimental and theoretical results on ionization of atoms, encapsulated into the fullerenes by photons with the energies of about 80-190eV. On the ground of…

Atomic Physics · Physics 2015-06-19 M. Ya. Amusia , L. V. Chernysheva , E. G. Drukarev

The vibrationally resolved spectra of the pyrene cation and doubly-dehydrogenated pyrene cation (C$_{16}$H$_{10}$$^{.+}$; Py$^+$ and C$_{16}$H$_{8}$$^{.+}$; ddPy$^+$) are presented. Infrared predissociation spectroscopy is employed to…

The formation of polycyclic aromatic hydrocarbons (PAHs) and their methyl derivatives occurs mainly in the dust shells of asymptotic giant branch (AGB) stars. The bands at 3.3 and 3.4 $\mu$m, observed in infrared emission spectra of several…

Solar and Stellar Astrophysics · Physics 2016-04-20 T. Monfredini , F. Fantuzzi , M. A. C. Nascimento , W. Wolff , H. M. Boechat-Roberty