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We have investigated the photo-stability of pristine and super-hydrogenated pyrene cations C$_{16}$H$_{10+m}^+, m = 0,6, \mathrm{\ or\ } 16$) by means of gas-phase action spectroscopy. Optical absorption spectra and photo-induced…

星系天体物理 · 物理学 2016-11-23 M. Wolf , H. V. Kiefer , J. Langeland , L. H. Andersen , H. Zettergren , H. T. Schmidt , H. Cederquist , M. H. Stockett

In the present contribution, I summarize a systematic study of ISO and Spitzer mid-IR spectra of Galactic regions and star forming galaxies. This study quantifies the relative variations of the main aromatic features inside spatially…

天体物理学 · 物理学 2008-02-19 F. Galliano

Using the AKARI, Wide-field Infrared Survey Explorer (WISE), Infrared Astronomical Satellite (IRAS), Sloan Digital Sky Survey (SDSS) and Hubble Space Telescope (HST) data, we investigated the relation of polycyclic aromatic hydrocarbon…

We performed mid-infrared spectroscopic observations of 18 local dusty elliptical galaxies by using the Infrared Spectrograph (IRS) on board Spitzer. We have significantly detected polycyclic aromatic hydrocarbon (PAH) features from 14 out…

天体物理学 · 物理学 2009-11-13 H. Kaneda , T. Onaka , I. Sakon , T. Kitayama , Y. Okada , T. Suzuki

A novel technique is employed for estimating attenuation curves in galaxies where only photometry and spectroscopic redshifts are available. This technique provides a powerful measure of particular extinction features such as the UV bump at…

宇宙学与河外天体物理 · 物理学 2015-05-13 Charlie Conroy

The abundance of polycyclic aromatic hydrocarbons (PAHs) in low- and high-metallicity galaxies has been widely discussed since the time when detailed infrared data for extragalactic objects were first obtained. On the scales of entire…

宇宙学与河外天体物理 · 物理学 2015-06-15 M. S. Khramtsova , D. S. Wiebe , P. A. Boley , Ya. N. Pavlyuchenkov

We present a charge distribution-based emission model that calculates the infrared spectrum of fullerenes (C$_{60}$). Analysis of the modelled spectrum of C$_{60}$ in various charge states shows that the relative intensity of the features…

星系天体物理 · 物理学 2023-04-25 Ameek Sidhu , A. G. G. M. Tielens , Els Peeters , Jan Cami

Observations with the Canadian Hydrogen Intensity Mapping Experiment (CHIME) have been used to measure the 21 cm intensity mapping auto power spectrum, at $z\sim 1$, over a frequency range from 608.2 MHz to 707.8 MHz at wavenumbers…

The fate of thymine upon excitation by ultraviolet radiation has been the subject of intense debate over the past three decades. Today, it is widely believed that its ultrafast excited state decay stems from a radiationless transition from…

We analyze low resolution Spitzer infrared (IR) 5-14 micron spectra of the diffuse emission toward a carefully selected sample of stars. The sample is composed of sight lines toward stars that have well determined ultraviolet (UV)…

星系天体物理 · 物理学 2022-02-02 Derck Massa , Karl D. Gordon , E. L. Fitzpatrick

Electronic decoherence processes in trans-polyacetylene oligomers are considered by explicitly computing the time dependent molecular polarization from the coupled dynamics of electronic and vibrational degrees of freedom in a mean-field…

量子物理 · 物理学 2015-06-03 Ignacio Franco , Paul Brumer

We consider a ballistic Mach-Zehnder interferometer for electrons propagating chirally in one dimension (such as in an integer Quantum Hall effect edge channel). In such a system, dephasing occurs when the finite range of the interaction…

介观与纳米尺度物理 · 物理学 2009-03-12 Clemens Neuenhahn , Florian Marquardt

Anharmonicity strongly influences the absorption and emission spectra of polycyclic aromatic hydrocarbon (PAH) molecules. Here, IR-UV ion-dip spectroscopy experiments together with detailed anharmonic computations reveal the presence of…

Clusters of polycyclic aromatic hydrocarbons (PAHs) have been proposed as candidates for evaporating very small grains, which are thought to be precursors of free-flying PAHs. Evaporation rates have been calculated so far only for species…

星系天体物理 · 物理学 2014-09-05 Julien Montillaud , Christine Joblin

With increasing energy the diamagnetic hydrogen atom undergoes a transition from regular to chaotic classical dynamics, and the closed orbits pass through various cascades of bifurcations. Closed orbit theory allows for the semiclassical…

混沌动力学 · 物理学 2007-05-23 T. Fabcic , J. Main , T. Bartsch , G. Wunner

We determine the electronic density of states for computationally-generated bulk samples of amorphous chalcogenide alloys As$_{x}$Se$_{100-x}$. The samples were generated using a structure-building algorithm reported recently by us ({J.…

材料科学 · 物理学 2018-06-01 Alexey Lukyanov , Jon C. Golden , Vassiliy Lubchenko

We report new correlations between ratios of band intensities of the 15-20 {\mu}m emission bands of polycyclic aromatic hydrocarbons (PAHs) in a sample of fifty-seven sources observed with Spitzer/IRS. This sample includes Large Magellanic…

星系天体物理 · 物理学 2015-10-14 M. J. Shannon , D. J. Stock , E. Peeters

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…

宇宙学与河外天体物理 · 物理学 2015-05-20 V. Lebouteiller , J. Bernard-Salas , D. G. Whelan , B. Brandl , F. Galliano , V. Charmandaris , S. Madden , D. Kunth

PAHs are known to be one of the carriers of the ubiquitous aromatic IR bands. The IR spectra of many objects show IR emission features derived from PAH molecules of different size. Still some of the characteristics of the emitting…

太阳与恒星天体物理 · 物理学 2014-09-05 Silvia Oettl , Stefan E. Huber , Stefan Kimeswenger , Michael Probst

Studying the anharmonicity in the infrared (IR) spectra of polycyclic aromatic hydrocarbons (PAHs) at elevated temperatures is important to understand vibrational features and chemical properties of interstellar dust, especially in the…