γλώσσες
Σελίδες
Νομικός
Explore all categories to find your favorite topic
Bending of starlight by stars (Gravitational microlensing) angular Einstein radius with ‘typical’ DS ~ 8.5 kpc and DL ~ 6.5 kpc Bending of starlight by stars (Gravitational…
Lecture 8: Stellar Nucleosynthesis and Chemical Evolution of The Galaxy • Chemical evolution of the Galaxy: • Star Formation • Nucleosynthesis in Stars • …
Agnieszka Janiuk N. Copernicus Astronomical Center, Warsaw Gamma Ray Bursts from Collapsing Massive Stars Collaborations: R. Moderski (CAMK), D. Proga(UNLV), Y. Yuan (ChAS),…
Search for neutrino bursts from gravitational collapse of stars at the Baksan Underground Scintillation Telescope Yu.F. Novoseltsev, M.M. Boliev, I.M. Dzaparova, M.M. Kochkarov,…
1 Marc Lachièze-Rey – Blois 2007 The cosmological constant Marc Lachièze-Rey APC Paris Λ Marc Lachièze-Rey – Blois 2007 The cosmological constant is not a problem…
1 SPATIALLY RESOLVED STIS SPECTRA OF BETELGEUSE’S UPPER CHROMOSPHERE AND CIRCUMSTELLAR DUST ENVELOPE A Lobel Harvard-Smithsonian Center for Astrophysics 60 Garden Street…
The Video Drift Method to Measure Double Stars Richard Nugent 33rd IOTA Annual Meeting Las Vegas, Nevada October 17, 2015 WHY MEASURE DOUBLE STARS ? Position angles (θ)…
Slingshot prominences evolution in Cool Stars CAROLINA VILLARREAL D’ANGELO MOIRA JARDINE ANDREW COLLIER CAMERON VICTOR SEE ROSE WAUGH Cool Stars 20 – Boston 2018 ΩΩ…
Modelling of W UMa-type Variable Stars Patricia Skelton MSc UNISA Prof. Derck Smits SKA Postgraduate Bursary Conference The Wallenberg Centre, stis 1 – 5 December 2008…
PETER TIBORIS | ΠΑΝΑΓΙΩΤΗΣ ΤΙΜΠΟΡΗΣ G E N E R A L D I R E C T O R | Γ Ε Ν Ι Κ Ο Σ ∆ Ι Ε Υ Θ Υ Ν Τ Η Σ FESTIVAL OF THE AEGEAN I N T E…
Astro Lingo Greek Letters are used for the names of bright stars within a constellation starting with α and for the names of constants and variables in equations Greek letter…
Slide 1CHARA Collaboration Year-Eight Science Review Host stars investigations with VEGA/CHARA R. Ligi, D. Mourard, A.-M. Lagrange, K. Perraut Observatoire de la Côte d’Azur,…
ΒΙΟΓΡΑΦΙΚΟ ΣΗΜΕΙΩΜΑ CURRICULUM VITAE HERMIS IATROU PROFFESSOR INDUSTRIAL LABORATORY NATIONAL AND KAPODISTRIAN UNIVERSITY OF ATHENS January 2016 CONTENTS…
UNSTABLE GALAXY MODELS ZHIYU WANG, YAN GUO, ZHIWU LIN, AND PINGWEN ZHANG Abstract. The dynamics of collisionless galaxy can be described by the Vlasov- Poisson system. By…
FanCam infrared parallax program is feasible •Resulting astrometric precision overall •x α: 1.3±0.7 µm 0.04”±0.02” •y δ: 1.3±0.8 µm 0.04”±0.02” •xy-averaged:…
CONVECTION AND DEFLAGRATIONS IN THE PROGENITOR STARS OF SUPERNOVAE SAMUEL JONES HEIDELBERG INSTITUTE FOR THEORETICAL STUDIES THU 10 NOV 2016 Kavli IPMU Tokyo STELLAR EVOLUTION…
Double Vision N ρ θ An Introduction to Double Star Observations David Lee What are Double Stars A binary star system is bound by gravitational force Star systems…
Slide 1 Be born slow or die fast Spin evolution of neutron stars with alignment and counteralignment S. Eliseeva, S. Popov, V. Beskin astro-ph/0611320 Slide 2 Neutron star…
Strange particles and neutron stars - experiments at GSI Outline: Probing dense baryonic matter (1-3 ρ0) The nuclear equation-of-state In medium properties of strange…
Katrien Uytterhoeven The Kepler space mission: New prospects for δ Sct, γ Dor, and hybrid stars Instituto de Astrofísica de Canarias, Tenerife NMSU, January 23, 2012 Uytterhoeven…