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
Book Volume: 624
DOI: 10.1051/0004-6361/201834600
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).
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://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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