This shareable PDF can be hosted on any platform or network and is fully compliant with publisher copyright.
Star-disk interactions in galactic nuclei.
This page is a summary of: The effect of gaseous accretion disk on dynamics of the stellar cluster in AGN, Proceedings of the International Astronomical Union, August 2014, Cambridge University Press,
DOI: 10.1017/s1743921315007644.
You can read the full text:
The following have contributed to this page
Physics of Plasmas
We show that a broad range of instabilities that drive pattern formation in dusty plasmas can be treated in terms of a common resonant instability phenomenon. This led us to consider the possible o...
Journal of Space Weather and Space Climate
We present new neutral mass density and crosswind observations for the CHAMP, GRACE, and GRACE-FO missions, filling the last gaps in our database of accelerometer-derived thermosphere observations....
Physics of Plasmas
Dipolarization fronts (DFs), which are mostly characterized by a sharp and transient increase in the normal component (northward) of the magnetic field in the magnetotail, are formed by the plasma ...
