Accretion disk versus jet orientation in H2O megamaser galaxies
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 (2019)
Publication Type: Journal article
Publication year: 2019
Journal
Book Volume: 624
DOI: 10.1051/0004-6361/201834600
Abstract
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).
Involved external institutions
Julius-Maximilians-Universität Würzburg
Germany (DE)
National Radio Astronomy Observatory (NRAO)
United States (USA) (US)
Max-Planck-Institut für Radioastronomie / Max Planck Institute for Radio Astronomy
Germany (DE)
Princeton University
United States (USA) (US)
National Sun Yat-sen University
Taiwan (TW)
Harvard University
United States (USA) (US)
Germany (DE)
National Radio Astronomy Observatory (NRAO)
United States (USA) (US)
Max-Planck-Institut für Radioastronomie / Max Planck Institute for Radio Astronomy
Germany (DE)
Princeton University
United States (USA) (US)
National Sun Yat-sen University
Taiwan (TW)
Harvard University
United States (USA) (US)
How to cite
APA:
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. https://dx.doi.org/10.1051/0004-6361/201834600
MLA:
Kamali, F., et al. "Accretion disk versus jet orientation in H2O megamaser galaxies." Astronomy & Astrophysics 624 (2019).
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