NGC 4936: abundant multi-phase medium in the central weak X-ray cool core and optically dark H I clouds in the group

arXiv:2610.10721 · astro-ph.GA · Submitted 2026-10-07 · Read on arXiv

astro-ph.GA

Submitted: 2026-10-07

Updated: 2026-10-07

Code: https://github.com/astropy/photutils-datasets

Terminology

• AGN — 21× in this paper · explained in 1 episode
• Core — 15× in this paper · explained in 2 episodes
• Abundance — 12× in this paper · explained in 1 episode
• Velocity Dispersion — 12× in this paper · explained in 2 episodes
• Metallicity — 11× in this paper · explained in 3 episodes
• Aperture — 10× in this paper · explained in 1 episode
• Trace — 8× in this paper · explained in 2 episodes
• Calibration — 6× in this paper · explained in 7 episodes
• Consistency — 2× in this paper · explained in 3 episodes
• Hubble Space Telescope — 2× in this paper
• AGN Feedback — 1× in this paper · explained in 1 episode
• Cooperation — 1× in this paper · explained in 2 episodes
• Multi-Unit Spectroscopic Explorer — 1× in this paper
• Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes
• Star Formation Rate (SFR) — 1× in this paper · explained in 5 episodes

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