For decades,
black holes have carried a simple reputation: cosmic vacuum cleaners that pull
in everything nearby and never let go. New observations suggest that picture is
incomplete, and a little too tidy.
Astronomers led by Dr. Noel Castro Segura at the
University of Warwick tracked a stellar-mass black hole system called Swift
J1727.8−1613 through a dramatic outburst that began in 2023. Using the European
Southern Observatory’s Very Large Telescope, the team watched as the black hole
pulled gas from a nearby companion star, the classic feeding behavior everyone
expects. But it also expelled large amounts of that material back out through
powerful jets and winds, and kept doing so even after the outburst had visibly
faded.
That’s the surprising part. Black hole activity is
usually judged by brightness, how much light the infalling matter gives off as
it heats up. This system kept expelling gas at roughly the same rate it was
consuming material even after it had dimmed to about one-hundredth of its peak
brightness. In other words, the black hole looked like it had gone quiet, but
it was still actively processing and returning matter to its surroundings.
The findings help settle a longer-running debate in
astrophysics about whether black holes eject material through jets (narrow,
fast-moving beams) or winds (broader, slower outflows), or both at once, and
under what conditions. Earlier work on a different system had suggested jets
and winds were mutually exclusive, only one active at a time. The Warwick
team’s data on J1727 offers a rare direct measurement showing outflow can
roughly match inflow even at low accretion rates, a number theorists need to refine
their models of how black holes shape the galaxies around them.
It’s a small but telling correction to a story we
thought we already understood: black holes aren’t just consuming machines.
They’re closer to a digestive system, taking in, processing, and returning a
surprising share of what they catch.
Source:
University of Warwick / ESO, published July 31, 2026, in Monthly Notices of the
Royal Astronomical Society.
Original paper: Optical outburst evolution of the transient black hole X-ray binary Swift J1727.8−1613: disc response to jet ejections and late-outburst emergence of powerful disc winds (arXiv preprint, MNRAS).

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