Multi-component emission line fitting of NGC 613 reveals bar-driven gas inflow along the dust lanes and an AGN-driven biconical ionised outflow aligned with the radio jet.
@doi [ ] 10.1051/0004-6361/201424523, https://ui.adsabs.harvard.edu/abs/2014A&A...572A..86A 572
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Optimising the analysis of emission lines in galaxies: the case of the MUSE TIMER galaxy NGC 613
Multi-component emission line fitting of NGC 613 reveals bar-driven gas inflow along the dust lanes and an AGN-driven biconical ionised outflow aligned with the radio jet.