for Astrophysics [email protected][email protected] October 7th, 2016 CfA Postdoc Symposium, Phillips Auditorium, Harvard/CfA/SAO, Cambridge , MA In collaborations with: Julia Lee (Harvard), Mike Nowak (MIT), In collaborations with: Julia Lee (Harvard), Mike Nowak (MIT), Randall Smith (SAO), Gerard Kriss (STSI) and et al. Randall Smith (SAO), Gerard Kriss (STSI) and et al. Photoionization Modeling Photoionization Modeling of Warm Absorbing Outflows of Warm Absorbing Outflows in Active Galactic Nuclei in Active Galactic Nuclei PG 1211+143
– Active Galactic Nuclei Unified Model – Ionized X-ray Absorbers in AGNs of Seyfert I Galaxies • X-ray Ionized Absorbers – Warm Absorbers (WAs) and Ultra-fast Outflows (UFOs) • Photoionization Modeling of Ionized Absorbers • Absorber Density Profile • Unification of WAs and UFOs • Conclusion
Unified Model (radio-loud & -quiet AGN, Seyfert I & II Galaxies) Beckmann & Shrader 2012, Active Galactic Nuclei Unified Models for AFNs Antonucci, ARA&A, 1993, 31, 473 Unified Schemes for AGNs Megan Urry & Padovani, 1995, PASP, 107, 803 Fanaroff–Riley class I Fanaroff–Riley class II
in AGNs of Seyfert I Galaxies Introduction Introduction Warm Absorbers Beckmann & Shrader 2012 (bbody + powerlaw + ∑ emis) x ∏ abs Hot Corona K-shell Iron Disk Black-body PG 1211+143
Modeling of Ionized Absorbers Photoionization Modeling of Ionized Absorbers Photoionization Code XSTAR (Kallman + 1996, 2004) Gas density Luminosity (0.0136-13.6 keV) Radius Column density Shell thickness Outflow velocity BH mass King & Pounds 2015; XMM-Newton & Suzaku (42 radio-quiet, Tombesi et al 2011; 51 AGN, Gofford et al. 2013)
Distribution (AMD): similar to Emission Measure Distribution (EMD) Absorber Density Profile Absorber Density Profile Tombesi + 2013 n(r) ~ r -1.4 density profile Behar 2009
Modeling of Ionized Absorbers Photoionization Modeling of Ionized Absorbers Photoionization Code XSTAR (Kallman et al 1996, 2004) Gas density Luminosity (0.0136-13.6 keV) Radius Column density Shell thickness Outflow velocity BH mass (Haring & Rix 2004) σ = 4.4 (Kormendy & Ho 2013) King & Pounds 2015; XMM-Newton & Suzaku (Tombesi et al 2011; Gofford et al. 2013)