PPT-Chemo-dynamics of galaxies with resolved stellar population

Giuseppina Battaglia Instituto de Astrofisica de Canarias Tenerife Credit ESO HHHeyer Credit ESOL Calçada Karachentsev et al 2014 Individual Red Giant Branch stars. Patricia . Sánchez-Blázquez. (UAM). Jairo. Mendez-Abreu (IAC). Sebastian F Sánchez (UNAM). Isabel Perez (UGR). Fabian Rosales-Ortega (UAM). And . the CALIFA collaboration. Resolved stellar . population. The Cosmic Time Machine. Astronomical telescopes can’t help viewing the past.. . Distance and time are always mixed in astronomical observations.. The finite speed of light means that we always see things after they have happened–a delay of 8 minutes for the Sun and about 12 billion years for the most distant galaxies we can observe. In other words,. the full SED (. from. UV to . far-IR. ) of galaxies to put . constraints. on. dust. . attenuation. and star formation . determinations. , . from. z=0 to z=2. The CIGALE code and . its. application to Herschel . 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?. Scott Croom. Julia Bryant. Joss Bland-Hawthorn. Disturbed Things Come in . small. packages. Jessica V. Bloom. Kinematics can uncover processes shaping galaxy evolution. Bloom et al., 2016 (submitted). . Ste. llar. . P. opulations . at intermediate redshift . S. urvey. w. ith . WEAVE. Bianca Poggianti – Angela . Iovino. (co-. Leads. ). o. n . behalf. of the . StePS. team . A. Mercurio, M. . diffuse X-ray emission – a survey of highly inclined disk galaxies. How is the emission correlated with galaxy properties?. How . are observations compared to simulations. ?. Nature of the emission – X-ray line spectroscopy. Transiting Exoplanets. Dainis Dravins. 1. , . Hans-Günter Ludwig. 2. ,. Erik Dahlén. 1. ,. Martin Gustavsson. 1. , . Hiva. Pazira. 1. . 1. . Lund Observatory, Sweden, . 2. . Landessternwarte. Astronomy C Event 2019. Stellar Evolution in Normal & Starburst Galaxies. Supported by NASA’s Universe of Learning STEM Network. . NASA’s Universe of Learning Network/CXC/NSO . Astronomy 2019 (Division C). Stellar Evolution in Normal & Starburst Galaxies. NASA Universe of Learning/CXC/NSO. https://www.universe-of-learning.org/. . . . . . . . . . http://chandra.harvard.edu/index.html. The astonishing variety of galaxies derived from a few structural types. Sec 1.3. Irregulars. = misfits in any class. Edwin Hubble . The Realm of the Nebulae . (1936. ). ‘. Tuning Fork’ classification scheme of galaxies. life appearance conditions. Call of interest. Hyper-Emblematic. project. P2IO. Expression of interest . Stellar and Planetary Formation . Keywords:. Structure and dynamics, Radiation, Magnetic fields,. 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 . R. Ellis & S. G. Djorgovski. Winter 2011. Class Logistics. All info, lecture notes, useful links, . homeworks. , exams, announcements, etc., will be on the class website:. http://www.astro.caltech.edu/~schenker/ay124.