Study of Ionized Gas in the Galaxy NGC6361
摘要
Abstract
We studied the spiral galaxy NGC 6361 using spectra from the spectrograph TDS in Caucasian Mountain Observatory of the Sternberg Astronomical Institute, Lomonosov Moscow State University, and the velocity field obtained on Fabry–Perot interferometer of SCORPIO-2 at the 6m telescope of the Special Astrophysical Observatory, Russian Academy of Sciences. In the course of the work we prepared data and plotted line-of-sight velocity curves. Additionally for the four HII-regions of the galaxy we determined gas ionization mechanism using the BPT-diagram and calculated their metallicity.