Study of Ionized Gas in The Galaxy NGC 6361
In this paper we studied the spiral galaxy NGC 6361 using spectrums from TDS in Caucasian mountain observatory and the velocity field obtained on Fabry - Perot interferometer of SCORPIO-2 in SAO RAS. In the course of work we prepared data, plotted radial velocity curves. Additionally for the four regions of the galaxy we determined gas ionization mechanism using the BPT-diagramm and their metallicity.
Authors
- Y. I. Kosareva
Institutions
- Lomonosov Moscow State University (RU)
Publication Details
- Published
- 2025-01-01
- DOI
- https://doi.org/10.15826/b978-5-7996-3986-0.25
- Primary Topic
- Galaxies: Formation, Evolution, Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 0.00