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Extended coronal line emission and new clues to a possible dual AGN in the merger J1356+1026

Merging luminous galaxies are ideal laboratories for studying some of the most extreme astrophysical phenomena. The local (z = 0.1232) obscured quasar J1356+1026 has two nuclei, North and South (J1356N and J1356S), but despite numerous efforts, J1356S had not yet been confirmed as an AGN. Based on t...

Ausführliche Beschreibung

Gespeichert in:
Hauptverfasser: Bianchin M., Ramos Almeida C., González-Martín O., Zanchettin M. V., Carneiro M., Pereira-Santaella M., Tadhunter C., Speranza G., García-Bernete I., Audibert A., Alonso-Herrero A., Rigopoulou D., Labiano A., Acosta-Pulido J. A., García-Burillo S.
Format: Artigo
Sprache:Inglês
Veröffentlicht: EDP Sciences 2026-05-01
Schriftenreihe:Astronomy & Astrophysics
Schlagworte:
ism: lines and bands
galaxies: active
galaxies: nuclei
quasars: general
Online-Zugang:https://www.aanda.org/articles/aa/full_html/2026/05/aa59271-26/aa59271-26.html
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