JWST, Subaru, and ALMA observations of HH 270 identify a new collimated jet closer to the source and show interactions between the shock-excited jet and the molecular outflow.
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JWST finds infrared counterparts for nearly all micro-Jy radio sources, with star formation explaining the radio output in roughly 79% of cases after accounting for non-linear luminosity relations.
citing papers explorer
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A Study of HH 270 with the James Webb Space Telescope
JWST, Subaru, and ALMA observations of HH 270 identify a new collimated jet closer to the source and show interactions between the shock-excited jet and the molecular outflow.
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PEARLS: JWST Counterparts of Micro-Jy Radio Sources in the NEP Time Domain Field. II. All Four Spokes
JWST finds infrared counterparts for nearly all micro-Jy radio sources, with star formation explaining the radio output in roughly 79% of cases after accounting for non-linear luminosity relations.