PPT-How Environment Affects Galaxy Metallicity:

Lessons from the Illustris Simulation Shy Genel Hubble Fellow Columbia University Genel 2016 ApJ in press arXiv160202773 How Environment Affects Galaxy Metallicity Lessons from the. 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)^. Michael Hayden (NMSU), Jo . Bovy. (IAS), Steve . Majewski. (. UVa. ), Jennifer Johnson (OSU), Gail . Zasowski. (JHU), Leo . Girardi. (. Padova. ), Carlos Allende-. Prieto. (IAC), Ana Garcia-Perez (. Metallicity. Relation at High . Redshifts. Stellar-mass . Metallicity. Relation at . ｚ～. １．. 4. Kouji. OHTA. 　（. Kyoto University. ）. K. Yabe. , F. . Iwamuro. , S. Yuma, M. Akiyama, N. Tamura, FMOS team et al.. galaxy group, Stephan Cristian Calderon. What is it?. The sombrero galaxy is a spiral galaxy with an unusually bright nucleus within the constellation Virgo . How far is it. The sombrero galaxy is approximately 29milion light years from earth. Prof. Gerhardt R Meurer. Galaxy evolution in a nutshell. Galaxy Evolution. 2. Time machines. The farther we peer. The farther back in time we see. Reveal cosmic history. Hubble: to < 1 . Gyr. after big bang. 23.1 Our Parent Galaxy. 23.2 Measuring the Milky Way. Early “Computers”. 23.3 Galactic Structure. 23.4 The Formation of the Milky Way. 23.5 Galactic Spiral Arms. Density Waves. 23.6 The Mass of the Milky Way Galaxy. metallicity. gradients . in disk galaxies from . integrated stellar populations. Patricia Sánchez-. Blázquez. . And the CALIFA collaboration. Evolution of the . metallicity. gradients in cosmological simulations. 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.. Here’s the mystery story we’ll unfold…. Fuzzy blobs in the sky – new solar systems, or “galaxies”?. Observational tests. Herschel’s map of the “universe” . (what we today know as just our Galaxy). 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 .  . An X-ray/UV Perspective. Edmund Hodges-. Kluck. Joel . Bregman. . University of Michigan. How do baryons cycle in and out of galaxies, and how does this impact galaxy evolution?. What happened to the “missing” baryons?. at High Redshift Universe. KenTaro. Motohara . (. IoA. , . Univsersity. of Tokyo). Gas Phase . Metallicity. Gas Phase . Metallicity. (Oxygen Abundance) is crucial to understand galaxy formation/evolution, as it traces the previous star formation history. . /Fe]. SNII . release. . most. . alpha. –. elements. . SNIa. . release. . most. Fe-. peak. . elements. Other. . proposed. . possibilities. (1) A variable IMF. (2) . Differential. . retention.