PPT-Stellar obliquities in

exoplanetary systems Josh Winn Simon Albrecht Roberto Sanchis Ojeda Teruyuki Hirano Andrew Howard John Johnson Geoff Marcy Bill Cochran Dan Fabrycky the Kepler . - 201 3 Welcome to Stellar Partner Program Our partner prog ram, aims at building a select group of Partners to work together as a team, to reach the next level of success in the field of data recov Bryce . Adelstein-Lelbach. , Louisiana State University. What is the Integrated Assembler?. The Integrated Assembler (IA) is an assembler built in to the Clang compiler driver. N. ot a separate binary like the GNU Assembler (GAS). 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. Mansi M. Kasliwal (Caltech). On behalf of the. PALOMAR TRANSIENT FACTORY. The Eventful Universe. March . 18, 2010. Why “Local” Universe?. 2. The Eventful Universe/ Kasliwal . Mar 18, 2010. Gravitational Waves: . Parallax is the apparent displacement of an object against the background when seen from two different perspectives.. Definition of Parallax. To measure the distance to a star, astronomers measure the parallax shift of the star using 2 points of view that are as far apart as possible-at opposite sides of Earth’s orbit.. 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.. 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. 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. 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. 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). . 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:. life appearance conditions. Call of interest. Hyper-Emblematic. project. P2IO. Expression of interest . Stellar and Planetary Formation . Keywords:. Structure and dynamics, Radiation, Magnetic fields,.