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. Galaxies. T.Naab. , P. Johansson, R. . Cen. , K. . Nagamine. , R. . Joung. . and J.P.O.. PPPL:, 19 Dec . 2012. ApJ.L.,. 658,710 . (2007) ApJ.,697, . 38 . (2009). ApJ.L.,699,L178 (. 2009. ). ApJ.,725,2312 . 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,. 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?. 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.. 1. /28. Important for transits (see next slides).. . Transit depth = [ . R. planet. (. λ. ,t. ) / . R. star. (. λ,t. ) ]. 2. Not so important for eclipses because the eclipse is a simple difference, and the stellar variability typically is slower than the eclipse: . I am resolved no longer to linger,. Charmed by the world’s delight,. Things that are higher, things that are nobler,. These have allured my sight.. I am resolved to go to the Savior,. Leaving my sin and strife;. Dainis . Dravins. – Lund . Observatory. , Sweden. www.astro.lu.se. /~. dainis. KVA. Towards the science case for E-ELT . HIRES. , Cambridge UK, September 2012. STELLAR SURFACES. … where starlight and stellar spectra originate. A first of its kind collaboration between:. Indiana Office of Community and Rural Affairs (OCRA). Indiana Housing and Community Development Authority (IHCDA). Indiana Department of Transportation (INDOT). JEFFREY HALL. LOWELL OBSERVATORY, FLAGSTAFF, AZ. Project Timeline. 1988 1992 1996 2000 2004 2008 2012 . Construction/early observing. Rebuild 1. Broad survey. Solar analog survey. Rebuild 2. A/D boundary. Presented at the . NAACCR Annual Conference. Quebec City. June 22, 2010. What are CP. 3. R Reports?. Cancer Program Practice Profile Reports. Developed by the Commission on Cancer. Web based . comparative reports . 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. life appearance conditions. Call of interest. Hyper-Emblematic. project. P2IO. Expression of interest . Stellar and Planetary Formation . Keywords:. Structure and dynamics, Radiation, Magnetic fields,. AKARI/IRC – perspective to SPICA. T. . Wada, . Y. . Ohyama. , . H. . Matsuhara. , . M. . Malkan. , . T. . Goto. , . E. . Egami. , . J.H. . Kim, C. Pearson, . H. . Inami. , . D. . Burgarella. , . T. . a Resolved by the Senate (the House of Representatives