Gas kinematics and stellar archaeology of the Seyfert galaxy NGC 5643

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Date
2020
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Abstract
In this work we derive stellar archaeology and kinematics of the central 400 pc of NGC 5643. The star formation history (SFH) reveals nuclear contribution of stellar populations older (20% older than 3.5 Gyr) and younger (60% younger than 320 Myr) as compared to the circumnuclear region. The [OIII] 5007 Å kinematics reveals the eastern ionization cone with an outflow (-60 km/s ≤ v ≤ 120 km/s). © The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union.
  1. Active Galatic Nuclei
  2. Outflows
  3. Stellar Populations
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https://www.scopus.com/inward/record.uri?eid=2-s2.0-85103564289&doi=10.1017%2fS1743921320004044&partnerID=40&md5=01e0ce2b3d356bd09ba7287d28812bb5
https://repositorio.maua.br/handle/MAUA/678
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