PPT-Chemical abundances near the surface of AGB stars

Shuya Ota Cyclotron Institute 2282020 Joint Nuclear amp Astrophysics Seminar Cyclotron Institute TAMU Quest to origins of elements Protondrip line Neutrondrip line Nuclearchart numbers are magic . 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 (. Abundances, atmospheres Abundances, interiors Accretion Adaptive optics Aeolian processes Aeronomy Asteroid AnneFrank Asteroid Braille Asteroid Ceres Asteroid Dactyl Asteroid Eros Asteroid Gaspra Aste 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. Fall 2014. . Lecture 10; November 6, 2014. Next Thursday!. Astro. 1 Observing Session (Optional, Just for Fun). WHEN: November 13. th. at 7-9pm . Same time Nov. 20. th. if the 13. th. is cloudy. 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). The Sun and the Stars. Stellar Lifecycle. Starbirth. Young Stars. Globular Clusters. Star Death. Star Death. Star Death. Star Death. Aims and Objectives. To introduce you to the properties of . t. he Sun and the stars, and their evolution. How are these two pictures related?. How to fold your paper…. Hold the paper lengthwise and fold the edges into the center.. Flip the paper over and write . Agree or Disagree . at the top.. Number 1-5 down the paper.. 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 A . star is a massive ball of plasma that emits . light and electromagnetic energy . throughout the universe. . While . there is only one star in our solar system, there are billions upon billions of stars throughout our galaxy and exponentially more in the billions of galaxies in the universe.