PPT-Understanding Metallicity

at High Redshift Universe KenTaro Motohara IoA Univsersity of Tokyo Gas Phase Metallicity Gas Phase Metallicity Oxygen Abundance is crucial to understand galaxy formationevolution as it traces the previous star formation history . Banks approach the DRT Securitization and Reconstruction of Financial Assets and Enforcement of Security Interests SARFAESI Act 2002 Borrowers guarantors and other any other person aggrieved by any action of the bank approach the DRT under the SARFA brPage 3br Understanding Heuristics Symantecs Bloodhound Technology Introduction The word heuristic was initially coined by the Greeks its original form was heuriskein which meant to discover Today the term is used almost exclusively in computer sci 50 years of Wide Field Studies, La Serena, 5/2013. 1. Robert Blum. Outline. History. The Galactic Bulge. Cosmology. Magellanic Clouds. 50 years of Wide Field Studies, La Serena, 5/2013. 2. Preliminaries. 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 (. Planet-Host Stars. 2013. 2. 22. . Wonseok. Kang . Kyung . Hee. University. Sang-. Gak. Lee. . Seoul National University. Why? : Abundances of Planet Host Stars. 2. Workshop on Stars, Planets, and Life 2013. “Education: That which discloses to the wise and disguises from the foolish their lack of understanding.”- Ambrose Pierce. Interpreted by Dr. Rich Hawkins and Dr. Deborah . DeLuca. Presented . By:Laura. metallicity. on pulsating B stars in the LMC (. Engelbrecht. , UJ):. UBVI photometry determines pulsation modes;. MOS spectroscopy (with SALT) determines . metallicity. .. Squares show all fields select for study (5 yellow fields completed). Diane Feuillet . New Mexico State University. Jon . Holtzman. , . Jo . Bovy. , Leo . Girardi. The APOGEE . Team. Thick disk:. Old. Kinematically. hot. Metal poor. Alpha rich. Thin disk:. Younger. Kinematically. Q: in order to study the spatial distribution of the thin disk (which dominates the Milky Way luminosity) surface photometry in the K band from space has been used. What is the advantage of the K band? What sort of stars give off most of their light at 2 microns. Steve . Goldman. 12 April, 2016. Cavendish Laboratories. AGB and RSG. Masers. SED fitting. Mass loss. The impact of the SKA. Asymptotic Giant Branch Stars . Understanding the mass loss and dust contribution of AGB and RSG to the ISM. Metallicity. Stellar Abundances: Victories and Struggles. Chris Sneden, University of Texas. speaking on behalf of . many . friends and colleagues in the stellar abundance & . nucleosynthesis. game. Laura . Magrini. INAF- . Osservatorio. . Astrofisico. di . Arcetri. In Our Galaxy. Open clusters (disc population): . Many (~2200 known clusters). . even more new candidates in the inner disc from infrared surveys . Ultra Metal - Poor (UMP ; [Fe/H] - 4 . 0 ) stars hold the key to the nucleosynthesis processes associated with first - generation stars in the Universe . However, only about two dozen UMP stars have b /Fe]. SNII . release. . most. . alpha. –. elements. . SNIa. . release. . most. Fe-. peak. . elements. Other. . proposed. . possibilities. (1) A variable IMF. (2) . Differential. . retention.