PPT-Mysterious Abundances in Metal-poor Stars & The

ν p process How do we explain the abundances of lighter heavy nuclei 38 Z 40 Sr Y Zr From Jacobson H R amp Frebel A 2014 Journal of Physics G Nuclear Physics 41 044001. stars. T. . Sivarani. . Indian Institute of Astrophysics, Bangalore. Chemical abundances of . metal poor stars. Probing the first stars – Stellar archeology. Looking for the fossil records of early star formation and Galaxy evolution . 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 (. 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 (. 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 Planet-Host Stars. 2013. 2. 22. . Wonseok. Kang . Kyung . Hee. University. Sang-. Gak. Lee. . Seoul National University. Why? : Abundances of Planet Host Stars. 2. Workshop on Stars, Planets, and Life 2013. 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). Way. Matthew Shetrone. University of Texas, McDonald Observatory. Giuseppina. . Battaglia. Instituto. de . Astrofisica. De Canarias. Jennifer . Johnson, . Joel . Zinn. Ohio State . University. Dennis . Elliptical Galaxies. Spiral Galaxies. Barred Spiral. Lenticular. Irregular (. L. arge . M. agellanic . C. loud). Dwarf Spheroidal Galaxy. Isochrone - 2.5x10. 8. yrs. Isochrone - 4x10. 9. yrs. IMF in the ρ Oph Association. SDSS. Timothy C. Beers. University of Notre Dame . First-generation objects of high mass presumably formed from . . metal-free gas. Lived short lives (. Myrs. not . Gyrs. ). Exploded. Distributed (pre or post explosion) their . 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). VEGA. . Recent. . results. and . ongoing. programs. CHARA 2017:. . Year 13 Science Review . –. Adaptive Optics and Open Access. The VEGA instrument. 4-beams visible combiner (3 in standard modes). Ultra Metal - Poor (UMP ; [Fe/H] - 4 . 0 ) stars hold the key to the nucleosynthesis processes associated with first - generation stars in the Universe . However, only about two dozen UMP stars have b : Parts I. Extremely. . metal-poor. (EMP) . stars as . probes of . earliest. . heavy. . elements. . nucleosynthesis. Abundance. . curve. in . solar. system & neutron capture . processes. Shuya Ota. Cyclotron Institute. 2/28/2020 . Joint Nuclear & Astrophysics Seminar, Cyclotron Institute, TAMU. Quest to origins of elements. Proton-drip line. Neutron-drip . line?. Nuclear-chart. (numbers are “magic” #).