Challenging the archetypal intermittent radio galaxy J0111+3906. New insights from optical GTC/OSIRIS and radio VLA and LOFAR observations

arXiv:2609.18543 · astro-ph.GA · Submitted 2026-09-16 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-16

Updated: 2026-09-16

Comments: 12 pages, 8 figures, accepted for publication in A&A

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Calibration — 21× in this paper · explained in 7 episodes
• AGN — 15× in this paper · explained in 1 episode
• Core — 15× in this paper · explained in 2 episodes
• Gran Telescopio CANARIAS — 3× in this paper
• Metallicity — 3× in this paper · explained in 3 episodes
• Very Large Array — 2× in this paper
• Accuracy — 1× in this paper · explained in 1 episode
• Alignment — 1× in this paper · explained in 1 episode
• Archetype — 1× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• Frustration — 1× in this paper · explained in 2 episodes
• Initial Mass Function (IMF) — 1× in this paper · explained in 2 episodes
• International LOFAR Telescope — 1× in this paper
• Star Formation Rate (SFR) — 1× in this paper · explained in 5 episodes
• Trace — 1× in this paper · explained in 2 episodes

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