Related publications
Papers presenting the observations, measurements, and physical interpretation connected to this work.
![Three processed emission maps shown side by side: Chandra 0.3–3 keV X-rays, ALMA CO (2–1), and VLT/MUSE Hα plus [N II], displayed with a blue-to-red intensity palette.](/_next/image?url=%2Fimages%2Fresearch%2Fngc5728-multiphase-emission-bands.png&w=3840&q=75)
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Research theme
Multiphase Galactic Outflows
I compare X-ray, molecular, and warm ionized gas observations to test whether spatially associated phases trace related outflow structures and how model-dependent energetics constrain possible feedback.
Scientific questions
Questions guiding this work
- 01
Where are X-ray, molecular, and warm ionized structures spatially associated, and what measurements would establish common motion or physical coupling?
- 02
How do measured morphology and kinematics differ among gas phases from nuclear to galactic scales?
- 03
Which observations and model-dependent energetics constrain possible energy and momentum transfer among gas phases and into the host?