- What are the connection(s) between outflows seen in X-ray absorption, in UV absorption, and at longer wavelengths?
- How do accretion structures (thin/slim/thick disk; chaotic cold accretion; etc.) depend on physical parameters?
- What impact do different accretion structures have on outflows?
- How important are continuum, line, and MHD driving to accelerating outflows?
- What signatures of wind acceleration should we look for (in X-rays, in the UV, etc)?
- What can continuum and absorption variability tell us about source and outflow properties and structure (e.g., will rotation + azimuthal asymmetries lead to UV absorption trough variability)?
- What are typical rates of mass, momentum, and kinetic energy loss via outflows?
22-26 May 2017
