Active Galactic Nucleus (AGN)

Active Galactic Nuclei (AGNs) are compact regions at the centers of galaxies that emit exceptionally high levels of electromagnetic radiation, often outshining the rest of the galaxy.

Active Galactic Nucleus (AGN)

Active Galactic Nuclei (AGNs) Latest News

Astronomers from the Russian Academy of Sciences, using the Spektr-RG (SRG) space observatory, have detected 11 new Active Galactic Nuclei (AGNs) during their all-sky X-ray surveys.

What are Active Galactic Nuclei (AGNs)?

  • Active Galactic Nuclei (AGNs) are compact regions at the centers of galaxies that emit exceptionally high levels of electromagnetic radiation, often outshining the rest of the galaxy.
  • This intense emission arises from either accretion of matter by a supermassive black hole or intense star formation activity.
  • AGNs are among the most luminous and persistent energy sources in the universe and are critical to understanding galaxy formation and evolution.
  • The newly detected AGNs were identified during an optical and X-ray inspection of sources listed in the ARTSS1-5 catalog, using SRG’s ART-XC telescope.
  • The team has also previously identified more than 50 AGNs and several cataclysmic variable stars.

Key Characteristics of the 11 Newly Detected AGNs

  • All 11 AGNs are located at redshifts ranging from 0.028 to 0.258, indicating they are relatively nearby in cosmic terms.
  • Their X-ray luminosities fall within the typical range of 2 to 300 × 10³⁹ erg/s, which is consistent with known AGN profiles.

Classification into Seyfert Types

  • All detected AGNs were classified as Seyfert galaxies, a type of AGN that is common and well-studied:
    • 7 galaxies were classified as Seyfert Type 1 (Sy 1), characterized by broad optical emission lines.
    • 3 galaxies were classified as Seyfert Type 1.9 (Sy 1.9), showing partially broadened lines.
    • 1 galaxy was classified as Seyfert Type 2 (Sy 2), which exhibits narrow emission lines only.
  • Seyfert galaxies appear like normal galaxies in visible light but show strong infrared and X-ray emissions due to activity at their cores.

Active Galactic Nuclei (AGNs) FAQs

Q1: What are Active Galactic Nuclei (AGNs)?
Ans: AGNs are extremely bright central regions of some galaxies, powered by supermassive black holes accreting matter.

Q2: Why are AGNs important in astrophysics?
Ans: AGNs help scientists understand galaxy evolution, black hole activity, and cosmic energy sources across the universe.

Q3: What types of AGNs are there?
Ans: Common types include quasars, blazars, Seyfert galaxies, and radio galaxies, each emitting energy across various wavelengths.

Source: PHY

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