ΔV⋆-g, a new stellar-gas kinematic mismatch parameter, shows no excess disturbance in MaNGA AGN compared to inactive controls.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Introducing $\Delta V_{\star-g}$: a new universal kinematic disturbance parameter
ΔV⋆-g, a new stellar-gas kinematic mismatch parameter, shows no excess disturbance in MaNGA AGN compared to inactive controls.