NGC 1068 deep millimeter spectroscopy observations Virtual Observatory Resource

Authors

1. Qiu J.
2. Wang J.
3. Shi Y.
4. Zhang J.
5. Fang M.
6. Li F.

Published by

CDS

Abstract

We aim for a better understanding of gas properties in the circum-nuclear disk (CND) region of the nearby gas-rich Seyfert 2 galaxy NGC 1068. We focus on line identification and the basic physical parameters estimation of molecular gas in the CND region. Methods. We used the IRAM 30m telescope to conduct deep millimeter spectroscopy observations toward the center of NGC 1068.

Keywords

1. active-galactic-nuclei
2. radio-spectroscopy

Bibliographic source Bibcode

2018A&A...613A...3Q

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/613/A3

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/613/A3

Document Object Identifer DOI

doi:10.26093/cds/vizier.36130003

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