Black Holes Can Trigger Gas to Collapse Into Stars

Jun 16, 2021 | Daily Space, Supermassive Black Holes

IMAGE: Virtual Milky Way: gas density around a massive central galaxy in a group in the virtual universe of the TNG50 simulation. Gas inside the galaxy corresponds to the bright vertical structure: a gaseous disk. To the left and right of that structure are bubbles – regions that look like circles in this image, with markedly reduced gas density inside. This geometry of the gas is due to the action of the super massive black hole that hides at the center of the galaxy and that pushes out gas preferably in directions perpendicular to the galaxy gaseous disk, carving regions of lower density. CREDIT: TNG Collaboration/Dylan Nelson

The Universe is a destructive place, and we like to remind folks that the Universe is always trying to kill us. Sometimes, however, things you might only expect to cause destruction can actually trigger creation. For instance, black holes. 

In new research appearing in the journal Nature and led by Ignacio Martín-Navarro, researchers describe how the flares and outbursts of supermassive black holes in the centers of large galaxies can clear the way for orbiting dwarf systems to form stars. Normally, these small, low-mass systems charge into the thin gas on the outskirts of massive galaxies and experience an effect called Ram Pressure Stripping. Essentially, it’s like holding a dandelion gone to seed out the window of a car and watching it get stripped of its fluff: the gas just pushes everything not held tightly out of the system. When black holes misbehave and outburst, however, they push all that thin gas out of the region above and below a galaxy, allowing the satellite galaxies in polar orbits to keep forming stars. 

So there you go. One black hole’s destruction means surviving star formation for passing dwarfs with just the right orbit.

More Information

Max Planck Institute press release

Anisotropic satellite galaxy quenching modulated by black hole activity,” Ignacio Martín-Navarro et al., 2021 June 9, Nature

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