H2$\lambda$2.4085 along the jet direction, the morphology of ionised The CO(2-1) line emission was found to be displaced by around 1 arcsec The continuum emissionĪt 237 GHz, though weak was found to spatially coincide with the AGN, however, Spectroscopic data suggest shock ionization of the gas. MAPPINGS, and estimation of temperature using Gemini and MaNGA integral field Modelling of the spectral lines using CLOUDY and The high resolution radio image and theĮxtended $\lambda$5007 emission, indicative of an outflow, are spatiallyĬoincident and are consistent with the interpretation of a low power radio jet Structures are situated on either side of the radio core that coincides with Structure is seen in the 15 GHz continuum image and the two asymmetric jet like Radio structure of $\sim$10 parsec size in NGC 4395. Here weĭemonstrate radio jet-ISM interaction on the scale of an asymmetric triple Spatial scales to which this feedback process can operate is unclear. Usually been on kiloparsec and larger scales and our knowledge on the smallest Such feedback processes, reminiscent of those seen in massive galaxies, haveīeen reported recently in some dwarf galaxies. May interact with their interstellar medium (ISM) affecting star formation. Download a PDF of the paper titled Evidence for low power radio jet-ISM interaction at 10 parsec in the dwarf AGN host NGC 4395, by Payel Nandi and 11 other authors Download PDF Abstract: Black hole driven outflows in galaxies hosting active galactic nuclei (AGN)
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