PPT-COS Abundances of

Nearby Star Forming Galaxies Alessandra Aloisi STScI Hot Science STScI 7 August 2013 COS Abundances of Nearby Star Forming Galaxies Alessandra Aloisi STScI. De Bievre and PDP Taylor Int J Mass Spectrom Ion Phys 123 149 1993 iiiiiiiiiiiiiiiiiiii Isotope Abundance iiiiiiiiiiiiiiiiiiii H 99985 H 0015 He 0000137 He 99999863 Li 75 Li 925 Be 100 10 B 199 11 B 801 12 C 9890 13 C 110 14 N 996 F F (4a) 1STDASampleARR 3 visible at some intermediate point will not be observable because the isotopic composition of the product must eventually duplicate that of the reactant. Second, since is abundances(Vazquezetal).Theseresultsstressthebenetsofadoptingacommunity-levelapproachthroughnetworkanalysis,asitallowsuncoveringpatternswhichwouldbeunobservableotherwise.Inthispaper,weanalysealargedat 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. – Dept. Physics and Astronomy University of . Hawai`i. Hilo. Daniel . Berke. . – James Clerk Maxwell Telescope . Forest Bremer . - Dept. Physics and Astronomy University of . Karl Young and Taryn Heilman. Astronomy 5022. December 4, 2014. Introduction. Two parameters affect abundances. n/p and η. Cosmological probe sensitive to the first 20 minutes of the universe. Predictions rely on GR and standard model so BBN probes these as well. 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 1 Hydrogen H 1.007825 99.9885 Deuterium H 2.014102 0.0115 Tritium H 3.016049 * 2 Helium He 3.016029 0.000137 He 4.002603 99.999863 3 Lithium Li 6.015122 7.59 Li 7.016004 92.41 4 Berylliu Solar System Abundances of the Elements Katharina Lodders Planetary Chemistry Laboratory, Dept. of Earth & Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, Campus 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 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. Raffaele . Gratton. INAF – . Osservatorio. . Astronomico. di . Padova. , ITALY. Contribution to GC science: numbers. 139 entries in ADS with "Cohen, J." AND "globular“:. oldest 1975, most recent 2016 (query on Jan. 11, 2017). 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).