PAH hypothesis Virtual Observatory Resource

Authors
  1. Pauzat F.
  2. Talbi D.
  3. Ellinger Y.
  4. Published by
    CDS
Abstract

IR spectra of anthracene and pyrene derivatives, serving as models for isolated, linear and isolated, compact PAHs, respectively, have been calculated using ab-initio quantum mechanical methods. The separate and combined effects of ionization and multiple dehydrogenation have been studied. This study confirms and refines the trends of our preliminary paper on the smallest possible PAH, naphthalene. If small PAHs are responsible for any UIR bands, they should be ionized and partially dehydrogenated, with a few triple bonds at the periphery of the carbon skeleton. In the appendix are given the complete IR spectra of all the isomers of the derivatives of anthracene and pyrene calculated for the purpose of this study. Tables I are for anthracene and Tables II for pyrene. Positions of the the missing hydrogens in the dehydrogenated species are referred as in Figures 1 and 2 of the original publication.

Keywords
  1. interstellar-medium
  2. infrared-astronomy
  3. spectroscopy
Bibliographic source Bibcode
1997A&A...319..318P
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/319/318
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/319/318
Document Object Identifer DOI
doi:10.26093/cds/vizier.33190318

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/319/318
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/319/318
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/319/318
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

1997-12-09T17:52:38Z
Resource record created
1997-12-09T16:52:54Z
Updated
1997-12-09T17:52:38Z
Created

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr