Black Hole 210
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Black Hole 210
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Nature
volume 601 , pages 329–333 ( 2022 ) Cite this article
Black-hole-driven outflows have been observed in some dwarf galaxies with active galactic nuclei 1 , and probably play a role in heating and expelling gas (thereby suppressing star formation), as they do in larger galaxies 2 . The extent to which black-hole outflows can trigger star formation in dwarf galaxies is unclear, because work in this area has previously focused on massive galaxies and the observational evidence is scarce 3 , 4 , 5 . Henize 2-10 is a dwarf starburst galaxy previously reported to have a central massive black hole 6 , 7 , 8 , 9 , although that interpretation has been disputed because some aspects of the observational evidence are also consistent with a supernova remnant 10 , 11 . At a distance of approximately 9 Mpc, it presents an opportunity to resolve the central region and to determine if there is evidence for a black-hole outflow influencing star formation. Here we report optical observations of Henize 2-10 with a linear resolution of a few parsecs. We find an approximately 150-pc-long ionized filament connecting the region of the black hole with a site of recent star formation. Spectroscopy reveals a sinusoid-like position–velocity structure that is well described by a simple precessing bipolar outflow. We conclude that this black-hole outflow triggered the star formation.
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The spectroscopic data analysed in this study are available from the Mikulski Archive for Space Telescopes (MAST) at https://archive.stsci.edu/.
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