Volume 486, Number 3, August II 2008
|Page(s)||L25 - L29|
|Published online||16 June 2008|
Letter to the Editor
The role of the charge state of PAHs in ultraviolet extinction
Istituto Nazionale di Astrofisica – Osservatorio Astronomico di Cagliari, Strada n. 54, Loc. Poggio dei Pini, 09012 Capoterra (CA), Italy e-mail: email@example.com
2 Centre d'Étude Spatiale des Rayonnements, Université de Toulouse – CNRS, Observatoire Midi-Pyrénées, 9 avenue du Colonel Roche, 31028 Toulouse Cedex 04, France
3 University College London, Department of Physics and Astronomy, Gower Street, London WC1E 6BT, UK
Accepted: 9 June 2008
Aims. We explore the relation between the charge state of polycyclic aromatic hydrocarbons (PAHs) and the extinction curve morphology.
Methods. We fit extinction curves with a dust model including core-mantle spherical particles of mixed chemical composition (silicate core, sp2 and sp3 carbonaceous layers), and an additional molecular component. We use exact methods to calculate the extinction due to classical particles and accurate computed absorption spectra of PAHs in different charge states, for the contribution due to the molecular component, along five different lines of sight.
Results. A combination of classical dust particles and mixtures of real PAHs satisfactorily matches the observed interstellar extinction curves. Variations of the spectral properties of PAHs in different charge states produce changes consistent with the varying relative strengths of the bump and non-linear far-UV rise.
Key words: ISM: dust, extinction / ISM: lines and bands / ultraviolet: ISM
© ESO, 2008
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.