S0 Galaxies: Outer Gas Accretion through Tidal Interaction and Minor Merging
Galaxies(2023)
Abstract
To clarify the sources of outer gas accretion onto disk galaxies, we study the vicinity of four interacting galaxy systems in the H alpha emission line by using the scanning Fabry-Perot interferometer of the 6m telescope of the Special Astrophysical Observatory RAS. We find perspective accretion flows seen as ionized-gas emission filaments between the galaxies. We discuss the whole kinematics and origin of these flows.
MoreTranslated text
Key words
disk galaxies,galactic structure,star formation,galaxies: kinematics and dynamics
AI Read Science
Must-Reading Tree
Example
![](https://originalfileserver.aminer.cn/sys/aminer/pubs/mrt_preview.jpeg)
Generate MRT to find the research sequence of this paper
Chat Paper
Summary is being generated by the instructions you defined