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Starburst regions in W-R gals composed of compact SSCs ... Underlying older population contributes to L(4861) 'continuum dilution' ...
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Wolf-Rayet Stars ... become Wolf-Rayet star is decreased for higher rotation ... A STRIKING OBSERVATIONAL FACTS. Very Helium-rich stars in Centuri ? DY/DZ ...
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Luminous Blue Variables. h Car. 100 x. more luminous. in the MIR. Wolf Rayet Stars. Luminous Blue Variables. WNL. N,He,H. WNE. N,He. WC. C, O. H (& He) Burning ...
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Wolf-Rayet in Spectrograph. Jupiter and Satellite in Slit Viewer. CorMASS (R=300) ... Spectrograph Camera. Grating. Tight Packaging to minimize Grating Turn Angle (30 ...
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Title: Iron-60 and Sun Formation Subject: Isotopes and Chronology Author: cosmoeye Keywords: star, Sun, iron, nickel, isotope, half-life, half-life, protoplanetary disk
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An Even More Precise View of Aluminum-26 in the Solar Nebula 26Al might have come from: Active stars before the Solar System formed, or Radiation of dust near the ...
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Evolved Massive Stars
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Spectro-photographie M thode d imagerie amateur au prisme-objectif Cyril Bazin A St L ger t 2000 Technique de prise de vue Mise en station Pointage et cadrage ...
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... (ESO, OHP, CTIO, VLA) and spaceborne (XMM-Newton, Chandra, INTEGRAL) facilities ... XMM-Newton and INTEGRAL studies of the X-ray and soft gamma-ray emission from ...
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Guidage et suivi manuel sur une toile guide. D veloppement manuel de ... 5 minutes de suivi balay , film TP2415 non hyper. Prisme de 30 plac devant Lunette 70 mm ...
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in spherically-symmetric winds, there should be no net polarisation. ... Here there are two winds: The polarisation amplitude is the total value for both ...
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... Katzman Automatic Imaging Telescope (KAIT) at Lick Observatory on Oct. 13, 2006. Swift Ultraviolet/Optical Telescope image of Supernova 2006jc in the galaxy UGC ...
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Electric field emitted from one atom which undergoes collisions: E n(t)= E0 cos(?0t fn (t) ... If there is laser emission, the coherence time of light is three or ...
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Semiconvection is the term applied to the slow mixing that goes ... Altair ( Aquilae) veq ' 230 km/sec. Teff4 / geff * tKH. Effects of rotation ...
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Linear spectropolarimetry. Jorick Vink (Armagh Observatory) Linear ... X ray emission. Questions for Star Formation. Do all stars form by disk accretion? ...
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M33 (3 fields) Phoenix. IC 10 IC 1613. NGC 6822 Sextans A. WLM Sextans B. How Are We Doing? ... Phoenix. WLM. What's Next? Spectroscopy! M31. N206 in M31. ob78 ...
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If DM is a fermion and coupled to heavy particles ... coupled to light particles (Z' ... Look like SUSY but relationship between the couplings and MF, ...
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5 out of 7 stars have essentially solar CNO abundances (weak 3rd dredge-up because of low mass? ... LS V 4621 (=Sh2-216): CNO and He 1-2 dex subsolar ...
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A Survey of Local Group Galaxies Currently Forming Stars
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Old population ( 2 Gyr): 4000 Ang break and other Lick indices. SSP: spectral evolution ... 5. Lick Indices : age/metallicity. CSF vs IB: RSG features. Mayya ...
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Title: Astronomy and Space Science Author: Alex Last modified by: sleung Created Date: 7/28/2006 9:51:18 AM Document presentation format:
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Once high mass stars are off the main sequence, they have different post MS ... High mass stars burn many elements and have 'onion-like' shells of material ...
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Massive star feedback from the first stars to the present Jorick Vink (Keele University)
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Ber rios Estelares : O Meio Interestelar e Forma o de Estrelas Helo sa Boechat GEA / Observat rio do Valongo / UFRJ
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F,G,K,M Stars. John Rayner (IRTF/IfA), Bill Vacca (Sofia-USRA) & Mike Cushing (Steward Obs.) 2 ... We have been using SpeX to construct an infrared ...
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LISA spectrograph Long slit Intermediate resolution Spectrograph for Astronomy Performances and application Christian Buil Active Spectroscopy in Astronomy
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What s new and what questions remain since our previous meeting? Workshop on Physics at the End of the Galactic Cosmic-ray Spectrum April 26-30, 2005
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Gamma ray bursts from binary black holes Agnieszka Janiuk Center for Theoretical Physics, Polish Academy of Sciences, Warsaw Collaboration: Szymon Charzy ski (Warsaw ...
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Supernovae, Gamma-Ray Bursts, and Stellar Rotation S. E. Woosley (UCSC) A. Heger (Univ. Chicago) The Neutrino Powered Wind Duncan, Shapiro, and Wasserman (1986) Qian ...
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thermal differentiation (e.g. melting, volatility) ... The abundance curve of the nuclei in the solar system comprises an average of ...
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Jet simulations and sources. Relativistic leptonic and hadronic ... SNs/SNRs: blast wave shock. Jet morphology. Jet simulation. M. Krause, LSW HD. t = 1.64 Myr ...
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... by treating cleveite with mineral acids. ... Cleveite is an impure ... cleveite. Pierre Jules. Janssen: 1824-1907. Lord Rutherford: 1871-1937. Helium ...
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... beam, a shocked cocoon, and a bow shock, and it is narrowly collimated ... with a cocoon surrounding the jet beam and a dense 'plug' at the head of the jet ...
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570 nm = 0,000570 mm = 7500 angstr ms. S miniare Aude Mai 2002. 6. Les raies spectrales ... Associer une longueur d'onde un pixel. S miniare Aude Mai 2002. 22 ...
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Astronomy C Event
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Code developed on the basis of hydrodynamic stellar structure equations for ... Goldreich-Schubert-Fricke instability: oscilatory instability due to temperature ...
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Utilisation des mesures de flux IR : I(?) ajustement un mod le thermique (distribution de temp rature) contrainte sur la taille de la source et l'albedo ...
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Title: Neutron star masses: dwarfs, giants and neighbors Author: PKSternberg Last modified by: sternberg pk Created Date: 11/26/2005 8:18:07 AM Document presentation ...
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The Orion Nebula is one of the most prominent. ... Were it not for the radiation of the O stars, the Orion Nebula would be invisible. ...
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ASSOCIATION D ASTRONOMIE V GA PLAISIR 78370 ... Binaires clipses : calcul des masses, ainsi que les rayons respectifs des composantes, ...
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Directly - apsidal motion of binaries - stars not point masses tidal torques ... Apsidal motion - stars not point masses so tidal torques cause precession of the ...
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... interstellar medium and in various other sites in the Galaxy, they trace stellar ... Correlation between galactic free-free emission and emission at 1.809 Mev ...
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GLAST Large Area Telescope: First Light
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as Long Gamma-Ray Burst progenitors Matteo Cantiello - Sterrekundig Instituut Utrecht What s this talk about? Rotation and Massive Stars Chemically Homogeneous ...
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Long Gamma Ray Bursts ( 2s): Death of Massive stars ... Fast rotating single massive stars could be long Gamma Ray Burst progenitors ...
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Astronomy & Astrophysics. Group Profile. Prof John Brown (Astronomer ... Dr Alec Mackinnon (Dept. of Adult & Cont. Educ.) Dr Graham Woan. Faculty: Research and ...
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Radiative Capture Experiments at ISAC
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This scenario is compatible with the aerogel model. ... The aerogel model is a robust model framework for understanding the SLRs ...
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Some dim stars have names according to their place in a catalogue (e.g. ... Just by looking, we cannot tell if a star is close and dim or far away and bright ...
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The Impact of the Galactic Center Arches Cluster: Radio & X-ray Observations ... Canto et al. (2000) predict such a wind. and simulations by Raga et al. (2001) ...
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A round or axisymmetric shape, sometimes with multiple shells or outer haloes. ... Silkworm. NGC 6302. Hb 5. Size does matter! 28. 28. A necessary question...
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... on stellar yields, which determine Galactic chemical evolution (superior goal) We further restrict to very hot, hydrogen-deficient, post-AGB stars.
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Gemini, Chile. Lick Obs., USA. NASA IRTF, USA. 8-m. 3-m. 3-m. opt.spectra, R=60000. CFHT, USA ... H line profiles are mostly double-peaked ...
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Protostars or Young Stellar Objects (YSO's) ... 'Live hard, die young, leave a good looking corpse' Peeling off to the Giant Phase ...
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