LeMMINGs III. The e-MERLIN legacy survey of the Palomar sample: Exploring the origin of nuclear radio emission in active and inactive galaxies through the [O iii] - Radio connection
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What determines the nuclear radio emission in local galaxies? We combine
optical [O III] line emission, robust black hole (BH) mass estimates, and
high-resolution e-MERLIN 1.5-GHz data, from the LeMMINGs survey, of a
statistically-complete sample of 280 nearby, optically active (LINER and
Seyfert) and inactive HII and Absorption line galaxies [ALG]) galaxies. Using
[O III] luminosity (
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1365-2966