PPT-Superbubble Driven Outflows in Cosmological Galaxy Evolution

Ben Keller McMaster University James Wadsley Hugh Couchman CASCA 2015 Paper astroph 150506268 Keller Wadsley amp Couchman 2015 Background Image Gas column density of IGM around a simulated . Driven Outflows in Cosmological Galaxy Evolution. Ben Keller (McMaster University). James . Wadsley. , Hugh . Couchman. CASCA 2015. Paper. : . astro-ph. : 1505.06268. Keller, . Wadsley. & . Couchman. Thorsten Naab . MPA, . Garching. . What regulates galaxy formation? . Leiden, April, 22. nd. How do massive galaxies get their gas and stars?. Gas accretion involves dissipation – energy can be radiated away . Reionization. by Early Galaxies. Brant E. Robertson, Richard S. Ellis, James S. Dunlop, Ross J. . McLure&Daniel. P. Stark, 'Early star-forming galaxies and the . reionization. of the Universe', Nature November 4, 2010 v 468 . Life in the Universe. Chapter 18. Life in the Universe. Units of Chapter 18. Cosmic Evolution. Life in the Solar System. Intelligent Life in the Galaxy. The Search for Extraterrestrial . Intelligence. Band Support. LTE:. 700/850/900/1800/2100/2600 MHz. UMTS:. 850/900/2100 MHz. GSM/EDGE: 850/900/1800/1900 MHz. Speed. LTE (4G): 150Mbps peak downlink rating. in limited areas. Actual speeds are less. Typical download speeds are 2Mbps – 50Mbps in all capital CBD’s (meaning with 5km from GPO), associated airports and approximately 80 regional locations (meaning within 3km from regional town centre)^. 134CHAPTER13.ASTROPHYSICALJETSwinds:jetsmightbepressure-driven,radiation-driven,Alfven-wave-driven,orshock-driven.Nooneissurehowjetsarecollimated;bythetimetheyarevisibletoobservers,theyarealreadytight outflows. : . 3C293 in 3D. Elizabeth . Mahony . (ASTRON, the Netherlands Institute for Radio Astronomy). Raffaella. . Morganti. (ASTRON, Univ. of Groningen). , Raymond . Oonk. (ASTRON). , Tom . Oosterloo. and . S6 Edge. March 2015 Cascade. Course Outline. Status Update: Pending Items as of March 19, 2015. Pricing .  . Closed (Go to Slide 13). Plans .  . Closed (please check S6 Queries Tracker). EPC Codes . Ketan Maheshwari. , Alex Rodriguez, David Kelly, Ravi . Madduri. , Justin Wozniak, Michael Wilde, Ian Foster. Argonne National Laboratory & University of Chicago. Overview. Introduce the Galaxy and Swift systems. ’ 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. Roberto Maiolino. Feedback is the key:. - reducing SF efficiency . . (gas . heating+turbulence. ). - removing baryons. Discrepancy . between halo . mass . functions . and stellar/baryons mass function. Contains more than 100 billion stars. Is one of the two largest among 40 galaxies in the Local Group. Our Solar System is located a little more than half way from the galactic center to the edge of the galactic disk.. 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. Driven Well Construction Features Assembled lengths of two inches to three inches diameter metal pipes are driven into the ground A screened well point located at the end of the pipe helps drive the