The IAU Commission X1 is a Cross-Division D-J initiative with the primary goal of promoting the development of research on supermassive black holes (SMBHs), active galactic nuclei (AGNs) and star formation feedback, as well as their role in galaxy evolution.
Through this commission, we aim to foster interaction between theorists and observers across the electromagnetic spectrum to investigate the interplay between the growth of SMBHs and galaxies, including the effects of their environment.
We aim to bridge the studies on feedback from the “galaxy evolution" community, which primarily focuses mostly on the role of star formation, and the “AGN" community, which concentrates on feedback from the environments of the nuclear SMBH, in order to advance our understanding of galaxy evolution.


We welcome input from the community to enhance our initiatives and collaborations. Please share your feedback by completing this form

News

NASA’s Hubble Identifies One of Darkest Known Galaxies

Using the NASA/ESA Hubble Space Telescope, astronomers have identified an exceptionally faint galaxy, known as Candidate Dark Galaxy-2 (CDG-2), that appears to be nearly invisible except for a few surrounding globular star clusters. By combining Hubble’s sharp imaging with data from ESA’s Euclid and the Subaru Telescope, researchers confirmed the presence of a diffuse glow indicating an underlying galaxy that is overwhelmingly dominated by dark matter, making it one of the darkest known galaxies ever discovered. This finding, enabled by advanced statistical techniques to detect faint structures, offers new insights into the hidden population of dark matter-rich galaxies in the nearby universe.

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An International Team of Astronomers Led by Umass Amherst May Have Just Found One of the Missing Links in Galaxy Evolution

An international team of astronomers has uncovered a previously unknown population of dusty, star-forming galaxies that existed just about one billion years after the Big Bang. These ancient galaxies, identified through a combination of ALMA’s submillimeter data and James Webb Space Telescope observations, may represent a “missing link” in the evolutionary sequence between ultrabright early galaxies and much older quiescent ones, challenging current models of how galaxies formed and evolved in the early universe.

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Conferences

Continuing the JWST Revolution: Understanding Early Galaxy Formation

01-26 June 2026

Continuing the JWST Revolution: Understanding Early Galaxy Formation workshop brings together observers and theorists to review early star/galaxy/black-hole formation, reionisation and future strategies with facilities like JWST, ALMA, SKA and ELT.

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Kyoto Torus Workshop 2026

18-22 May 2026

TORUS 2026: Multi‑wavelength approach to the AGN structures focuses on advancing our understanding of AGN structures — especially the torus — by combining multi‑wavelength observations and realistic physical models, with fresh insights from XRISM, JWST, ALMA, and simulations.

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Papers

Disentangling multiple gas kinematic drivers in the Perseus galaxy cluster

XRISM Collaboration, Nature, 650, 309-313, 2026

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Evidence of Feedback Effects in Low-luminosity Active Galactic Nuclei Revealed by JWST Spectroscopy

Zhang L., Packham C., Hicks E. K. S. et al., ApJL, 998, L32, 2026

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