'Light days' presentation slideshows

Quasar Structure: Why the details matter for Co-evolution

Quasar Structure: Why the details matter for Co-evolution. Martin Elvis Harvard-Smithsonian Center for Astrophysics. Simulation. Bimodal galaxy colors. Data. AGN & Galaxy Evolution. Example: AGN winds, radiation inhibit star formation? Bimodal galaxy colors in GOODS

721 views • 53 slides

Getting it all together: Paradigms for AGNs

562 views • 43 slides

Outflows in AGN: High and Low Resolution X-ray View

Outflows in AGN: High and Low Resolution X-ray View. Yair Krongold (IA-UNAM). Fabrizio Nicastro (OAR-INAF) Elena Jimenez-Bailon (IA-UNAM) Martin Elvis (CfA) Nancy Brickhouse (CfA) Luc Binette (IA-UNAM) Smita Mathur (OSU). Warm Absorbers = AGN Winds.

267 views • 26 slides