Search results for Signatures of Peculiar Supernova Nucleosynthesis in ... Galactic metal-poor stars with [Fe/H] < -1 Old stars that were formed 10 Gyrs ago Mostly enriched by core-collase SNe (CCSNe)

MNRAS 000, 1–31 (2018) Preprint 5 July 2018 Compiled using MNRAS LATEX style file v3.0 Testing Gravity with wide binary stars like α Centauri Indranil Banik1∗ and Hongsheng…

Evidence from the Motions of Old Stars that the Galaxy Collapsed O J Eggen D Lynden-Bell and A R Sandage 1962 ApJ No 136 p 748 Presented by: Michael Solway All equations…

Binary Stars and Fundamental Stellar Parameters PHY 521 Lecture 26 Dec 6 2011 PHY 521 Lecture 26 2 Mass • most fundamental of stellar parameters – L ∝ M38 – τMS…

Probing the Galactic Potential Using the μarcsec astrometric observations of Disk Stars T. 　　Sumi　　　 (Nagoya STE) K.V. 　Johnston (Columbia) S.　　　Tremaine…

High Resolution Imaging of dust disks structures around Herbig Ae stars with VISIR C.Doucet, P-O Lagage, E. Pantin (CEA Saclay SAp) E. Habart (IAS, Orsay) C. Pinte, G. Duchêne,…

ar X iv :1 70 7 04 00 6v 4 as tr o- ph S R 2 7 D ec 2 01 7 MNRAS 000 1–15 2017 Preprint 29 December 2017 Compiled using MNRAS LATEX style file v30 LAMOST Views δ Scuti…

Neutrino-Nucleus Reaction Cross Sections for Neutrino Detection and Nucleosynthesis in Supernova Explosions Toshio Suzuki Nihon University INPC 2016 Sept 15 2016 ・ New…

Neutrinos in Cosmology II Sergio Pastor IFIC Valencia 29th Indian-Summer School of Physics, Prague 4-8 Sep 2017 ν ν ν ν ν ν ν ν ν ν ν ν ν ν ν ν ν ν ν ν…

14 may 2007Simbol-X workshop - Bologna1 44 Ti nucleosynthesis γ –ray lines with Simbol-X Matthieu Renaud Max-Planck-Institute für Kernphysik Heidelberg, Germany Collaborators:…

Stars Zombies Οι ελληνικές επιχειρήσεις βγαίνοντας από την κρίση wwwpwccomgr Μάιος 2014 Ανάπτυξη για την Ελλάδα…

Debris Disk Evolution Mark Wyatt Institute of Astronomy Cambridge What are debris disks Planetesimals and dust found around ~15% of main sequence stars The planetesimals…

1 6 Stellar spectra excitation and ionization Saha’s equation stellar spectral classification Balmer jump H- 2 Occupation numbers: LTE case Absorption coefficient: κν…

THE MAGNUS METHOD FOR SOLVING OSCILLATORY LIE-TYPE ORDINARY DIFFERENTIAL EQUATIONS MARIANNA KHANAMIRYAN Department of Applied Mathematics and Theoretical Physics, University…

A method for modelling high-order, g-mode pulsators: The case of γ Doradus stars. A. Moya Instituto de Astrofísica de Andalucía – CSIC, Granada, Spain Brief introduction…

A method for modelling high-order, g-mode pulsators: The case of γ Doradus stars. A. Moya Instituto de Astrofísica de Andalucía – CSIC, Granada, Spain Brief introduction…

Slide 1 Variable Stars: Pulsation, Evolution and applications to Cosmology Shashi M. Kanbur SUNY Oswego, June 2007 Slide 2 Stellar Evolution Recall equations of stellar structure.…

Habitable Zones around Evolved Stars Lee Anne Willson Iowa State University April 30, 2014 STScI 1 AU is in the habitable zone for our Sun, now. The planetary temperature…

Spectrophotometric properties of the nearest pre-main sequence stars 2009. 10. 07 A-Ran Lyo HR diagram Luminosity Temperature Pre-main sequence Lyo et al. 2004a Hα emission…

Slide 1 Nicolas Lodieu SAAO, 28 September 2005 Low-mass stars and brown dwarfs in open clusters Slide 2 The BD group @ Leicester  Head: Richard Jameson  Post-docs:…

Dark Matter in the Center of the Milky Dark Matter in the Center of the Milky Way and the Stars Burning ItWay and the Stars Burning It Igor V. Igor V. MoskalenkoMoskalenko…