Accretion disk versus jet orientation in H2O megamaser galaxies

Beitrag in einer Fachzeitschrift


Details zur Publikation

Autorinnen und Autoren: 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
Zeitschrift: Astronomy & Astrophysics
Jahr der Veröffentlichung: 2019
Band: 624
ISSN: 1432-0746


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).


Einrichtungen weiterer Autorinnen und Autoren

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


Zitierweisen

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).

BibTeX: 

Zuletzt aktualisiert 2019-17-04 um 07:33