Magellanic cloud PNe in the IR Virtual Observatory Resource

Authors

1. Stanghellini L.
2. Garcia-Lario P.
3. Garcia-Hernandez D.A.,Perea-Calderon J.V.
4. Davies J.E.
5. Manchado A.
6. Villaver E.
7. Shaw R.A.

Published by

CDS

Abstract

We present 5-40um spectroscopy of 41 planetary nebulae (PNe) in the Magellanic Clouds, observed with the Infrared Spectrograph on board the Spitzer Space Telescope. The spectra show the presence of a combination of nebular emission lines and solid state features from dust, superimposed on the thermal IR continuum. By analyzing the 25 LMC and 16 SMC PNe in our sample we found that the IR spectra of 14 LMC and four SMC PNe are dominated by nebular emission lines, while the other spectra show solid state features.

Keywords

1. magellanic-clouds
2. planetary-nebulae

Bibliographic source Bibcode

2007ApJ...671.1669S

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/671/1669

IVOA Identifier IVOID

ivo://CDS.VizieR/J/ApJ/671/1669

Document Object Identifer DOI

doi:10.26093/cds/vizier.16711669

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https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/671/1669/PNe?
https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/671/1669/PNe?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/671/1669/PNe?