Extended CO structures in NGC6240

DOI

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.

Cone search capability for table J/A+A/549/A51/table1 (Measured quantities from the uv-plane fit, and derived quantities (line luminosities and gas masses) of the CO-emitting components)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35490051
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/549/A51
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/549/A51
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/549/A51
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/549/A51
Provenance
Creator Feruglio C.; Fiore F.; Maiolino R.; Piconcelli E.; Aussel H.; Elbaz D.,Le Floc'h E.; Sturm E.; Davies R.; Cicone C.
Publisher CDS
Publication Year 2013
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; High Energy Astrophysics; Natural Sciences; Observational Astronomy; Physics