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Slide 1Roger Caballero-Folch (DFEN –UPC) València, 15 de juliol de 2013 β-decay half-lives and β- delayed neutron emission measurements for r-process nucleosynthesis…
Big Bang Nucleosynthesis (BBN) Eildert Slim Timeline of the Universe Baryon Asymmetry Baryon abundance parameter ηB = (nB - n ̅B)/nγ ηB very small: η10 = 1010 ηB Matter-antimatter…
Lecture 10 Nucleosynthesis During Helium Burning and the s-Process So typical temperatures are 2 x 108 K higher in shell burning later when densities are over 1000 gm cm-3…
Slide 1 Radio-quiet Isolated Neutron Stars (RQINs) Jeng-Lwen, Chiu Institute of Astronomy, NTHU 2004/09/30 Slide 2 Outline n Neutron stars n AXPs & SGRs n CCOs n XDINs…
Lecture 9 Hydrogen Burning Nucleosynthesis, Classical Novae, and X-Ray Bursts red = slow , , , I I j jk L k kj j k k j L L k I j dY Y Y I Y Y L dt ρ λ ρ λ ∍ + = + =…
Slide 1 Somak Raychaudhury www.sr.bham.ac.uk/~somak/Y2SiU/ Two-body problem Binary stars Visual Eclipsing Spectroscopic How to find extrasolar planets…
MNRAS 489, 1379–1396 2019 doi:10.1093mnrasstz2104 Advance Access publication 2019 August 2 Uncertainties in νp-process nucleosynthesis from Monte Carlo variation of reaction…
σ(E) = S(E) e–2πη E-1 2πη = 31.29 Ζ1Ζ2 √μ/Ε μ = m1m2 / (m1+m2) Reaction Rate(star) ÷ ∫Φ(E) σ(E) dE Gamow Peak Maxwell Boltzmann Extrap. Meas.σ Carlo Broggini…
1 ----- Ταχ. Δ/νση: Ανδρέα Παπανδρέου 37 Τ.Κ. – Πόλη: 15180 Μαρούσι Ιστοσελίδα: www.minedu.gov.gr Πληροφορίες:…
Study of 17O(p,α)14N reaction via the Trojan Horse Method for application to 17O Nucleosynthesis Maria Letizia Sergi LNS-INFN, Catania 53-esimo Congresso della Societa'…
NMR spektroskopie pevného stavu (1)(1) jirijiri brusbrus +1 +3 +2 0 −1 −2 −3 t1 τ 90°-sel. +1 +3 +2 0 −1 −2 −3 t1 τ 90°-sel. Přehled kursu ss-NMR spektroskopie…
Slide 1Ubatuba November 2005 2nd CoRoT Brazil δ Scuti and γ Dor stars in COROT Rafael Garrido IAA, Granada (Spain) Slide 2 Ubatuba Nov 20052nd CoRoT Brazil Current ground…
Slide 1 Toulouse May 2005 Corot-Week 8 δ Scuti and γ Dor stars in COROT Rafael Garrido IAA, Granada (Spain) Slide 2 Toulouse May 2005Corot-Week 8 Current ground based observations…
ar X iv :1 60 3 04 99 4v 1 as tr o- ph S R 1 6 M ar 2 01 6 MNRAS 000 1–39 2015 Preprint 17 March 2016 Compiled using MNRAS LATEX style file v30 The R136 star cluster dissected…
Early stars and galaxies : reionization of the Universe A Doroshkevich MDemianski Astro Space Centre of Lebedev Physical Institute University of Warsaw Progress in cosmology…
Experimental Investigation of the Reactions 25Mgαn28Si 26Mgαn29Si 18Oαn21Ne and their Impact on Stellar Nucleosynthesis Dissertation zur Erlangung des Grades Doktor der…
Slide 1 Atmospheric tomography of supergiant stars (starring μ Cep) Alain Jorissen, Sophie Van Eck, Kateryna Kravchenko (Université Libre de Bruxelles) Andrea Chiavassa…
FREE PRESSTimes ΔΕΚΑΠΕΝΘΗΜΕΡΗΕΝΗΜΕΡΩΤΙΚΗΕΦΗΜΕΡΙΔΑ ΤΗΣΘΕΣΣΑΛΙΑΣ τα δικά µας free νέα! AΡ ΦΥΛΛΟΥ 104-17 OKTΩΒΡΙΟΥ…
Light and Stars ASTR 2110 Sarazin Doppler Effect Frequency and wavelength of light changes if source or observer move Doppler Effect € vr ≡ dr dt ≡ radial…
The Future Summary: Dark Energy and Cosmic Fate Ωtot = 1 ΩΛ = 07 Trending: exp Λ312 t Gravity Dark Energy Λ ≈ 10-122 ! Long-term Cosmic Outcomes What do you expect…