PPT-IGRINS for Stellar Abundances & Nucleosynthesis

Chris Sneden Natalie Gosnell Dan Jaffe Greg Mace Richard Seifert UT Austin Hwihyun Kim IGRINS team members KASI Melike Afşar Ege U Izmir Turkey Caty Pilachowski Indiana U. MESSENGER SAX & RHESSI. Brian Dennis. 31 October 2012. Mercury MESSENGER. Solar Assembly for X-rays (SAX). Si-PIN solid-state. 300 µm thick. 1 to 10 keV. ~300 . eV. resolution at 6 keV. 0.12 mm. 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 (. . atmospheres. a . very. . short. . introduction. Part I. Ewa Niemczura. Astronomical. . Institute. , . UWr. eniem@astro.uni.wroc.pl. Stellar. spectra. Stellar. spectra. One picture is worth 1000 words, but . 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 (. Abundances, atmospheres Abundances, interiors Accretion Adaptive optics Aeolian processes Aeronomy Asteroid AnneFrank Asteroid Braille Asteroid Ceres Asteroid Dactyl Asteroid Eros Asteroid Gaspra Aste Icarus Key Words Abundances, interiors Accretion Adaptive optics Aeronomy Asteroid AnneFrank Asteroid Braille Asteroid Ceres Asteroid Dactyl Asteroid Eros Asteroid Gaspra Asteroid Ida Asteroid Itokaw 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. Soroush Sotoudeh. . (University of Minnesota). Daniel . Weisz. , Andrew Dolphin, Evan Skillman. 06/29/2015 – . STScI. Workshop on IMF. Outline. Introduction. Observations and data. IMF analysis and results. Guillermo A. Blanc. Universidad de Chile. OUTLINE. MEASURING ABUNDANCES IN IONIZED GAS. SEL METHOD SYSTEMATICS AND CHALLENGES. IZI: THE BAYESIAN APPROACH. THE ABUNDANCE SCALE DISCREPANCY. CONCLUSIONS. Transiting Exoplanets. Dainis Dravins. 1. , . Hans-Günter Ludwig. 2. ,. Erik Dahlén. 1. ,. Martin Gustavsson. 1. , . Hiva. Pazira. 1. . 1. . Lund Observatory, Sweden, . 2. . Landessternwarte. 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. Donald D. Clayton\'s Principles of Stellar Evolution and Nucleosynthesis remains the standard work on the subject, a popular textbook for students in astronomy and astrophysics and a rich sourcebook for researchers. The basic principles of physics as they apply to the origin and evolution of stars and physical processes of the stellar interior are thoroughly and systematically set out. Clayton\'s new preface, which includes commentary and selected references to the recent literature, reviews the most important research carried out since the book\'s original publication in 1968. . constraints. : AGB . stars. and . grains. S.Palmerini. AGB . stars. , . s-process. and . presolar. . grains. :. the story so far. Molecular Cloud. Meteorite. Presolar. grains. Despite their low masses LMS are so numerous to contribute for 75% to the total mass return from stars to the ISM (. Boris Pritychenko. 1. 1 National Nuclear Data Center, Brookhaven National. Laboratory, Upton, NY 11973-5000, USA. Heavy Elements Production in a Neutron Star Merger. Can we apply nuclear data libraries to address current astrophysical observations such as a multi-messenger signal from the NGC 4993 galaxy? .