activity
20142024
most citedPolycyclic Aromatic Hydrocarbons with armchair edges and the 12.7 μm band

42 citations · 118 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA20248 cited

Laser-induced fragmentation of coronene cations

S. Panchagnula, J. Kamer, A. Candian +4

Polycyclic aromatic hydrocarbons are an important component of the interstellar medium of galaxies and photochemistry plays a key role in the evolution of these species in space. H…

astro-ph.GA202410 cited

Photofragmentation of Corannulene (C20H10) and Sumanene (C21H12) cations in gas phase and its Astrophysical implications

P. Sundararajan, A. Candian, J. Kamer +2

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 ar…

astro-ph.GA2024

A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk

Olivier Berné, Emilie Habart, Els Peeters +143

Most low-mass stars form in stellar clusters that also contain massive stars, which are sources of far-ultraviolet (FUV) radiation. Theoretical models predict that this FUV radiati…

astro-ph.GA202421 cited

The Infrared Absorption Spectrum of Phenylacetylene and its Deuterated Isotopologue in the Mid- to Far-IR

Vincent J. Esposito, Piero Ferrari, Wybren Jan Buma +4

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

astro-ph.GA2016

High-resolution IR absorption spectroscopy of polycyclic aromatic hydrocarbons in the 3 μm region: Role of periphery

Elena Maltseva, Annemieke Petrignani, Alessandra Candian +5

In this work we report on high-resolution IR absorption studies that provide a detailed view on how the peripheral structure of irregular polycyclic aromatic hydrocarbons (PAHs) af…

astro-ph.GA201537 cited

The 11.2 m emission of PAHs in astrophysical objects

A. Candian, P. J. Sarre

The 11.2 m emission band belongs to the family of the `Unidentified' Infrared (UIR) emission bands seen in many astronomical environments. In this work we present a theoretical…