PPT-Microphysics and X-ray Spectra of AGN Outflows

T Kallman NASAGSFC Line emission efficiency across the spectrum Thermal stability The broadband spectrum of active galaxies flat over 68 decades Very different from stars Most are strong Xray sources. jdx or NIST msp format The spectra preferably should include 2 digits to the right of the decimal see Correcting for Mass SufficiencyDeficiency below The NIST program then uses two files to import the saved spectra The primary file AUTOIMPMSP is foun Molecular Outflows in Low- and High-MassStar-forming RegionsH Largest commercial flooring contractor. in U.S.. Over . 30 locations . nationwide. Over . 350,000 projects . in our portfolio. Large . bonding. capacity, solid . credit. lines, and national . buying. multitemperature. approach. . B. Sylwester, J. Sylwester, A. Kępa. . Space . Research. Centre, PAS, Wrocław, Poland. K.J.H. Phillips. Natural . History. . Museum. , London, UK. . V.D. . Kuznetsov. outflows. : . 3C293 in 3D. Elizabeth . Mahony . (ASTRON, the Netherlands Institute for Radio Astronomy). Raffaella. . Morganti. (ASTRON, Univ. of Groningen). , Raymond . Oonk. (ASTRON). , Tom . Oosterloo. Outflowing. Galactic Winds at . z. = 1. Katherine A. Kornei (UCLA). Alice Shapley, Crystal Martin, Alison Coil. ETH Zurich. . February 2012. Yang, M.-J., and R.A. . Houze. , . Jr. RTF. Hydrometeor types. Ice-phase microphysics. Environmental humidity. No. 1 microphysics processes. CNTL. Full model physics for 15 h. . Turn off the hail generation processes after 6 h (. ’ in the wind: . feedback from QSO outflows at high-z. Text by. : . G. Cresci. , . A. Marconi, M. . . Brusa. , . V. . . Mainieri. , S. . Carniani. , . M. . Perna. . et al. . Music by. : . B. Dylan. during November . 12-15, . 2015 and November 16-19, 2015. Robert Conrick, Qi Zhong, and Cliff Mass. University of Washington. . Pacific NW Weather Workshop 2017. Cases: November . 12-15, . 2015. protostellar. cores?. Chat Hull. University of California, Berkeley (USA). Radio Astronomy Laboratory. 5. February 2013. Session: Magnetic Fields in the ISM and Star-forming Regions I. Magnetic Fields in the Universe IV. cloud microphysics scheme in CAM. Hugh Morrison and Andrew . Gettelman. National Center for Atmospheric Research. CCSM Atmospheric Model Working Group Meeting. Feb 12, 2008. Thanks to Steve . Ghan. (PNNL). Ben Keller (McMaster University). James . Wadsley. , Hugh . Couchman. CASCA 2015. Paper. : . astro-ph. : 1505.06268. Keller, . Wadsley. & . Couchman. 2015. Background Image: Gas column density of IGM around a simulated . Seyfert. Galaxies Ark 564 and . Mrk. 590. Anjali. Gupta. Columbus State . Ohio State University. Collaborators: . Smita. . Mathur. , . Yair. . Krongold. Low velocity outflows are ubiquitous. . Hua Leighton. Collaborators: Robert Black, Frank Marks,. . . Xuejin. Zhang, . Gopal. . Sundararaman. Why do we care about microphysics?. Direct impact . . .