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Resource Record Summary

Catalog Service:
IR spectroscopy of PAH in 6-15{mu}m band

Short name: J/ApJ/729/94
IVOA Identifier: ivo://CDS.VizieR/J/ApJ/729/94
DOI (Digital Object Identifier): 10.26093/cds/vizier.17290094
Publisher: CDSivo://CDS[Pub. ID]
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/729/94
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2012 Oct 25 12:24:18Z
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Description


Polycyclic aromatic hydrocarbon (PAH) growth and destruction are thought to proceed via the occasional incorporation of five- and seven-membered fused ring defects in the hexagonal carbon skeleton. Using density functional theory, this paper investigates the effect such five- and seven-membered fused ring defects have on the infrared spectra of ovalene (OV; C_32_H_14_), circumovalene (c-OV; C_66_H_20_), and circumcircumovalene (cc-OV; C_112_H_26_). The defects make only small changes to the overall infrared (IR) spectra, both in the mid-IR and in the far-IR, of these species. In addition to small shifts in the positions of the bands between the PAHs with and without defects, the most common effect of the defects is to increase the number of bands. Except for an anion with the Stone-Wales defect, all of the species studied have the C-C stretching band at 6.3um or at longer wavelengths, the position in Classes B and C astronomical PAH spectra. In the case of the Stone-Wales anion, the band falls at 6.20um, suggesting that further study of defects is probably worthwhile, as some PAHs with defects might be important in those sources (Class A) that show a C-C stretching band that falls near 6.2um.

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About the Resource Providers

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Publisher: CDSivo://CDS[Pub. ID]

Creators:
Ricca A.Bauschlicher C.W.JRAllamandola L.J.

Contact Information:
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Email: cds-question at unistra.fr
Address: CDS
Observatoire de Strasbourg
11 rue de l'Universite
F-67000 Strasbourg
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Status of This Resource

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Version: n/a
Availability: This is an active resource.
  • This service provides only public data.
Relevant dates for this Resource:
  • Updated: 2012 Nov 14 10:39:04Z
  • Created: 2012 Oct 25 12:24:18Z

This resource was registered on: 2012 Oct 25 12:24:18Z
This resource description was last updated on: 2021 Oct 21 00:00:00Z

What This Resource is About

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Resource Class: CatalogService
This resource is a service that provides access to catalog data. You can extract data from the catalog by issuing a query, and the matching data is returned as a table.
Resource type keywords:
  • Catalog
Subject keywords:
  • Atomic physics
  • Interstellar medium
  • Astronomical models
Intended audience or use:
  • Research: This resource provides information appropriate for supporting scientific research.
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/729/94 Literature Reference: 2011ApJ...729...94R

Related Resources:

Other Related Resources
TAP VizieR generic service(IsServedBy) ivo://CDS.VizieR/TAP [Res. ID]
J/A+A/527/A109 : Dust and PAH emission SEDs of disk galaxies (Popescu+, 2011) ivo://CDS.VizieR/J/A+A/527/A109 [Res. ID]

Data Coverage Information

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Rights and Usage Information

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Available Service Interfaces

Custom Service

This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.

VO Compliance: Level 2: This is a VO-compliant resource.
Available endpoints for this service interface:
Custom Service

This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.

VO Compliance: Level 2: This is a VO-compliant resource.
Available endpoints for this service interface:
  • URL-based interface: http://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/729/94
Table Access Protocol - Auxiliary ServiceXX

This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.

VO Compliance: Level 2: This is a VO-compliant resource.
Available endpoints for the standard interface:
  • http://tapvizier.cds.unistra.fr/TAPVizieR/tap


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under Cooperative Agreement AST0122449 with the Johns Hopkins University
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