WebMay 5, 2016 · 1. INTRODUCTION. The mid-infrared spectra of many astronomical objects are dominated by the 3.3, 6.2, 7.7, 8.6 and 11.2 μm emission bands, which are generally attributed to the infrared (IR) fluorescence of polycyclic aromatic hydrocarbons (PAHs) that are pumped by the absorption of ultraviolet (UV) photons.These molecules contain some … WebMay 16, 2024 · Shubhadip Chakraborty 1 , Giacomo Mulas 1 2 , Karine Demyk 1 , Christine Joblin 1 Affiliations 1 Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse (UPS), CNRS, CNES , 9 Av. du Colonel Roche , 31028 Toulouse Cedex 4 , …
Christine Joblin - Wikiwand
WebRapacioli, Fernand Spiegelman, Christine Joblin To cite this version: Sébastien Zamith, Jean-Marc l’Hermite, Léo Dontot, Linjie Zheng, Mathias Rapacioli, et al.. WebChristine Joblin Cesare Cecchi-Pestellini View Computational investigation of the effects of perfluorination on the charge-transport properties of polyaromatic hydrocarbons Article Full-text... royalty free punk
Photo-dissociation of naphthalene dimer cations stored in a …
WebOct 24, 2024 · Deciphering the aromatic infrared bands: the LAIBrary project (Jean Jaurès) - Christine Joblin 17:40 - 18:00 The 3.4 µm absorption band profile : comparison of aliphatic interstellar dust observations and laboratory analogues properties (Jean Jaurès) - … WebChristine Joblin is a French astrochemist who uses spectroscopy to study photodissociation and the polycyclic aromatic hydrocarbons in cosmic dust.[1][2] Beyond … WebChristine Joblin è un'astrochimica francese che usa la spettroscopia per studiare la fotodissociazione e gli idrocarburi aromatici policiclici nella polvere cosmica. Oltre al suo lavoro sperimentale e di osservazione, ha anche contribuito alla prima chiara scoperta di ... royalty free punk rock