HCOOCH3 map of Orion-KL Virtual Observatory Resource

Authors

1. Favre C.
2. Despois. D
3. Brouillet N.
4. Baudry A.
5. Combes F.
6. Guelin M.,Wootten A. Wlodarczak G.

Published by

CDS

Abstract

The Orion Kleinmann-Low nebula (Orion-KL) is a complex region of star formation. Whereas its proximity allows studies on a scale of a few hundred AU, spectral confusion makes it difficult to identify molecules with low abundances. We studied an important oxygenated molecule, HCOOCH3, to characterize the physical conditions, temperature, and density of the different molecular source components.

Keywords

1. molecular-clouds
2. interstellar-medium
3. radio-astronomy

Bibliographic source Bibcode

2011A&A...532A..32F

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/532/A32

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/532/A32

Document Object Identifer DOI

doi:10.26093/cds/vizier.35320032

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/532/A32
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/532/A32
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/532/A32

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

Web browser access HTML

https://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/A+A/532/A32