The origin of past nuclear activity in galaxy GSN 069, a source of quasi-periodic X-ray eruptions (QPEs), has been investigated. Using polarimetry and spectropolarimetry with VLT/FORS2 on September 6, 2019, an increase in optical polarization from ~0% near the nucleus to ~1.5% in the periphery was detected, confirming the presence of an extended emission-line region (EELR). The rise in polarization points to a 'switched-off' nucleus. The polarization direction aligns with the axis of elongated emission in [OIII], [NII], and Hα lines, matching relic polarization cones and implying a past toroidal structure. Optical polarization echoes geometrically support a faded active galactic nucleus (AGN) scenario as the source of the EELR, although an enhanced rate of tidal disruption events (TDEs) cannot be entirely ruled out.
At the heart of every galaxy slumbers a supermassive black hole. When it devours matter, its surroundings flare up—this is an active nucleus. How can we learn about past outbursts if the black hole is silent? The answer lies in light echoes.
Like an echo in an empty hall, where reverberations linger after the source has gone quiet, radiation from a dead nucleus wanders through the galaxy. Astronomers caught it by measuring polarization—the orientation of light wave oscillations. In GSN 069, polarization grew stronger with distance from the center and was almost absent at the core. This means the light source has gone dark, but reflected rays still carry its story.
A combined analysis of spectroscopy and photometry revealed that the nucleus of GSN 069 wasn't just tearing apart passing stars—it shone steadily, surrounded by a gas 'doughnut' that focused its radiation. Most surprising: the black hole fell silent when ancient civilizations already existed on Earth. Its current slumber is just a brief pause in a turbulent life.
🎯 Light echoes expose cosmic events with a delay that makes us witnesses of the distant past—as if we're watching a film shot thousands of years ago.