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April 13, 2026Moscow University Physics Bulletin0 citations

Observations of Ionized Gas around Active Galaxies at the 2.5-m CMO SAI MSU Telescope

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ASA. A. SmirnovaAMA. V. MoiseevAAA. Arshinova

Key Points

  • The research aims to analyze ionized gas clouds influenced by active galactic nuclei and their effects on surrounding galaxies.
  • Utilized MaNGaL, a tunable filter narrow-band photometer, at the 2.5-m CMO SAI MSU telescope
  • Tracked AGN ionization cones in various galaxies
  • Mapped external emission filaments near NGC 1142/1144
  • Focused on observing fading activity and cross-ionization in interacting galaxies
  • Identified fading nuclear activity in merging galaxies
  • Observed cross-ionization effects in disc companions of galaxies
  • Generated the first [OIII] map for a rare object type known as ‘green beans’
  • Documented extensive ionization cones at redshifts z=0.2 to 0.4

Abstract

MaNGaL (Mapper of Narrow Galaxy Lines) is a tunable filter narrow-band photometer installed at the 2. 5-m telescope of the Caucasian Mountain Observatory of the Sternberg Astronomical Institute at Lomonosov Moscow State University (CMO SAI MSU). It enables us to detect and study the gas clouds, ionized by UV-radiation from an active galactic nucleus (AGN). We present a brief overview of MaNGaL observations of various manifestations of AGN ionization cones: tracking of fading nuclear activity in merging galaxies; the cross-ionization of disc companion of galaxies; the discovery of a complex system of external emission filaments near the NGC 1142/1144, the first OIII map of a rare type of objects known as ‘‘green beans, ’’ characterized by powerful, extended ionization cones at redshifts z=0. 2-0. 4.

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Cite This Study

Smirnova et al. (2025) studied this question.

synapsesocial.com/papers/69dc87983afacbeac03e9d94https://doi.org/10.3103/s0027134925701784
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