Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-28T16:54:44.916Z Has data issue: false hasContentIssue false
  • English
  • Français

Photophysics of interstellar PAHS+ in the PIRENEA experiment

Published online by Cambridge University Press:  25 September 2002

M. Giard ,
J.P. Bernard ,
A. Klotz ,
I. Ristorcelli ,
C. Pech ,
P. Boissel ,
M. Armengaud ,
P. Frabel  and
C. Joblin
C. Pech
Affiliation:
CESR, CNRS et Université Paul Sabatier, BP. 4346, 31028 Toulouse Cedex 04, France
P. Boissel
Affiliation:
LCP, CNRS et Université Paris Sud, Bât. 350, 91405 Orsay Cedex, France
M. Armengaud
Affiliation:
CESR, CNRS et Université Paul Sabatier, BP. 4346, 31028 Toulouse Cedex 04, France
P. Frabel
Affiliation:
CESR, CNRS et Université Paul Sabatier, BP. 4346, 31028 Toulouse Cedex 04, France
C. Joblin
Affiliation:
CESR, CNRS et Université Paul Sabatier, BP. 4346, 31028 Toulouse Cedex 04, France
Get access

Abstract

This paper reports the first results obtained on thephotodissociation of the isolated PAH cations 12C24H+12,13C12C23H+12 and 12C24H+10, usingthe astrochemistry experimental set-up PIRENEA.The dissociation patterns of these ions involvethe loss of pairs of hydrogen atoms. A first interpretation indicates that the-H2 dissociation path is favoured compared to the -H path in ourexperimental conditions. These results might have important implicationson the formation of H2 in the interstellar medium.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 4: Infrared and Submillimeter Space Astronomy: An International Colloquium to Honor the Memory of Guy Serra , 2002 , pp. 297
Copyright
© EAS, EDP Sciences, 2002

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)