PPT-Stellar-mass

Metallicity Relation at High Redshifts Stellarmass Metallicity Relation at ｚ １ 4 Kouji OHTA 　 Kyoto University K Yabe F Iwamuro S Yuma M Akiyama N Tamura FMOS team et al. Driven Outflows in Cosmological Galaxy Evolution. Ben Keller (McMaster University). James . Wadsley. , Hugh . Couchman. CASCA 2015. Paper. : . astro-ph. : 1505.06268. Keller, . Wadsley. & . Couchman. H.-W. Rix IMPRS Galaxies Course March 11, 2011. Goal:. Determine . n. *. (M. *. ,. t. age. ,[Fe. /H],. R. ). . for a population of galaxies. How many stars of what mass and metallicity . formed when and where in galaxies?. versus convective . blueshifts. , and wavelength variations across stellar disks. Dainis Dravins. – Lund . Observatory. , Sweden. www.astro.lu.se. /~. dainis. KVA. IAU Comm.30, IAU XXVIII GA Beijing, August 2012. Giuseppina. . Battaglia. Instituto. de . Astrofisica. de Canarias, Tenerife. Credit. : ESO/. H.H.Heyer. Credit. : ESO/L. . Calçada. Karachentsev. et al. 2014. Individual . Red . Giant Branch . stars. . Technique. . for. . the. . Determination. . of. IMF . at. . Low. . Masses. : . A. . Few. . Results. . for. . Galaxies. . with. Old. . Stellar. . Populations. Nikolay. Podorvanyuk. 1. Key variable is . mass. of star. directly measured only for binary stars, but it determines position on main sequence. Cluster ages. Main-sequence luminosity increases . much. faster than mass. therefore massive stars use up their fuel much faster. Steven R. . Cranmer. Harvard-Smithsonian Center for . Astrophysics. . with A. van . Ballegooijen. , S. Saar, A. Dupree, N. . Brickhouse. , et al.. Stellar winds across the H-R Diagram. Massive stars: radiation-driven winds. Revision . lecture. Lecture slides available in . powerpoint. and . pdf. from. www.star.le.ac.uk. /~. mbu. /. lectures.html. Everything taught in the course is examinable…... However, here is a crib sheet of what to focus on. Transiting Exoplanets. Dainis Dravins. 1. , . Hans-Günter Ludwig. 2. ,. Erik Dahlén. 1. ,. Martin Gustavsson. 1. , . Hiva. Pazira. 1. . 1. . Lund Observatory, Sweden, . 2. . Landessternwarte. Insights from recent surveys. Gaspard . Duchêne. (UC Berkeley, Obs. Grenoble). © NASA/JPL/Caltech. Planets in multiple systems?. © . LucasFilm. Ltd.. They must exist!. Planets in multiple systems!. 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 . . Matt Crouch.  . Project Manager. Kathleen . Weissenberger. State CDBG Director. Indiana Office of Community and Rural Affairs. 2014 Regional Conference. Indiana’s Stellar Communities. A first of its kind collaboration between:. N. . Prantzos. Lecturer:. . Hans-Jürgen . Wollersheim. e-mail: . h.j.wollersheim@gsi.de. web-page: . https://web-docs.gsi.de/~. wolle/. and click on . thermodynamics. subatomic physics. Sun´s energy. CIERA postdoctoral fellow. the stellar progenitors of long-duration gamma ray bursts. MICRA 2023. ECT*, Trento, IT. september 10, 2023. iron core. (stripped) stellar envelope. gravitational collapse.