Active galactic nuclei, energetic and luminous regions powered by an accreting supermassive black hole at the center of some galaxies, can launch a jet that drives a gas outflow, shaping star formation in their host galaxy. Justin Kader and colleagues have observed this phenomenon in the nearby active galaxy VV 340a. Kader et al. observed the jet and galaxy across infrared, optical, radio, and sub-millimeter wavelengths, using the James Webb Space Telescope, Keck-II telescope, the Jansky Very Large Array and the Atacama Large Millimeter/submillimeter Array. The researchers combined these observations with modeling, to show that the low-power radio jet emitted by VV 340a undergoes a conical wobble, known as precession, as it moves outward. The jet ionizes and ejects gas as it propagates away from the supermassive black hole, driving a gas outflow at a rate of 19.4 ± 7.9 solar masses per year. This outflow rate is large enough to affect the star formation rate of the host galaxy, Kader et al. conclude.

Active galactic nuclei, energetic and luminous regions powered by an accreting supermassive black hole at the center of some galaxies, can launch a jet that drives a gas outflow, shaping star formation in their host galaxy. Justin Kader and colleagues have observed this phenomenon in the nearby active galaxy VV 340a. Kader et al. observed the jet and galaxy across infrared, optical, radio, and sub-millimeter wavelengths, using the James Webb Space Telescope, Keck-II telescope, the Jansky Very Large Array and the Atacama Large Millimeter/submillimeter Array. The researchers combined these observations with modeling, to show that the low-power radio jet emitted by VV 340a undergoes a conical wobble, known as precession, as it moves outward. The jet ionizes and ejects gas as it propagates away from the supermassive black hole, driving a gas outflow at a rate of 19.4 ± 7.9 solar masses per year. This outflow rate is large enough to affect the star formation rate of the host galaxy, Kader et al. conclude.

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