Research area
Testing where AGN outflows heat, ionize, or redistribute gas from the nucleus across nearby host galaxies.
Observational approach
I compare resolved X-ray, optical emission-line, radio, and molecular-gas structures across nuclear, circumnuclear, and kiloparsec scales to locate measurable changes in the host-galaxy gas.
Observatories
Physical interpretation
Ionization or morphological alignment identifies an AGN influence, but galaxy-scale feedback requires evidence that the nucleus changes the gas distribution, dynamics, or energy budget.
Scientific questions
Where do observations indicate that AGN activity may heat, ionize, or redistribute gas in the host galaxy?
Which properties of the host regulate whether a nuclear wind produces measurable galaxy-scale effects?
Which tracers preserve evidence of accretion-driven structures from nuclear to kiloparsec scales?
Selected work
