Accretion disk versus jet orientation in H2O megamaser galaxies

Journal article

Publication Details

Author(s): Kamali F, Henkel C, Koyama S, Kuo CY, Condon JJ, Brunthaler A, Reid MJ, Greene JE, Menten KM, Impellizzeri CM, Braatz JA, Litzinger E, Kadler M
Journal: Astronomy & Astrophysics
Publication year: 2019
Volume: 624
ISSN: 1432-0746


Context. An essential part of the paradigm describing active galactic nuclei is the alignment between the radio jet and the associated rotation axis of the sub-pc accretion disks. Because of the small linear and angular scales involved, this alignment has not yet been checked in a sufficient number of low luminosity active galactic nuclei (LLAGNs).

External institutions with authors

Harvard University
Julius-Maximilians-Universität Würzburg
Max-Planck-Institut für Radioastronomie / Max Planck Institute for Radio Astronomy
National Radio Astronomy Observatory (NRAO)
National Sun Yat-sen University
Princeton University

How to cite

Kamali, F., Henkel, C., Koyama, S., Kuo, C.Y., Condon, J.J., Brunthaler, A.,... Kadler, M. (2019). Accretion disk versus jet orientation in H2O megamaser galaxies. Astronomy & Astrophysics, 624.

Kamali, F., et al. "Accretion disk versus jet orientation in H2O megamaser galaxies." Astronomy & Astrophysics 624 (2019).


Last updated on 2019-17-04 at 07:33