Extended CO structures in NGC6240 Virtual Observatory Resource

Authors

1. Feruglio C.
2. Fiore F.
3. Maiolino R.
4. Piconcelli E.
5. Aussel H.
6. Elbaz D.,Le Floc'h E.
7. Sturm E.
8. Davies R.
9. Cicone C.

Published by

CDS

Abstract

We present deep CO(1-0) observations of NGC6240 performed with the IRAM Plateau de Bure Interferometer (PdBI). NGC6240 is the prototypical example of a major galaxy merger in progress, caught at an early stage, with an extended, strongly-disturbed butterfly- like morphology and a heavily obscured active nucleus in the core of each progenitor galaxy.

Keywords

1. seyfert-galaxies
2. radio-astronomy

Bibliographic source Bibcode

2013A&A...549A..51F

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/549/A51

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/549/A51

Document Object Identifer DOI

doi:10.26093/cds/vizier.35490051

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