Confirmed Participants . ... Participants . ... Last updated:10:54:49 17-Jun-2015 . ...

... Title . Speaker . Moderator . Theories for the First Stars and First Clusters . ... Detectability of the First Stars and Massive Star Clusters . ... Evolution of the Early IGM . ... The Evolution of Galaxies . ... Star Formation . ... Astro-Chemistry in Dense Protostellar Environments . ... Star Formation Initial Mass Functions I : In "Normal" Galactic Environments . ... Star Formation Initial Mass Functions II: In Extreme Environments . ... Planetary System Formation and Evolution . ...

... We have examined the diversity of planets and planetary systems that arise from oligarchic growth and gas accretion onto massive cores, by means of N-body simulations combined with a sophisticated disc model. ... Slow planetary growth resulted from the relatively low mass of solids in the disc, and one consequence of this is that planets underwent limited orbital migration during the lifetime of the gas disc. ... Figure 1 shows an example of this migration behaviour in a single-planetin-a-disc run. ...

Main Program Travel Where to go in Moscow Information . ... The 2014 year marks the 100th anniversary of Yakov Zeldovich . ... John Carlstrom (University of Chicago) . ... Lyman Page (Princeton University) . ... The conference will be held at the Space Research Institute (IKI) in Moscow, Russia, on June 16-20, 2014 . ... International Conference: Cosmology and High Energy Astrophysics (Zeldovich-90) 20-24 Dec 2004, Moscow, Russia . ... 2014 Space Research Institute, Moscow Русская версия ...

... System E+FWCMS Program. ... Maria-Rosa Cioni (confirmed) - "The Magellanic Clouds as a template for the study of stellar populations and galaxy interaction" . Chiara Mastropietro (confirmed) - "Ram-pressure induced star formation in the LMC" . Akiko Kawamura (confirmed) - "Study of molecular clouds and star formation in the Magellanic Clouds" . ... Lynn Redding Carlson Dating Young Stellar Objects in the Magellanic Clouds . Annapurni Subramaniam Small Magellanic Cloud: A smaller halo? ...

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... Companion of a Young, Sun-like Star Confirmed . ... Toronto ) Explanation: The first direct image of an extrasolar planet orbiting a star similar to our Sun has been confirmed. ... This sharp infrared image shows the young star's planetary companion positioned above and left of center. ... The discovery image, shown above , was taken in 2008 but confirmed only recently by noting that the planet stayed with its parent star as background stars slightly shifted over time. ... NASA Official: Jay Norris....

... 2010 July 4 . Companion of a Young, Sun-like Star Confirmed . ... Explanation: The first direct image of an extrasolar planet orbiting a star similar to our Sun has been confirmed. ... This sharp infrared image shows the young star's planetary companion positioned above and left of center. ... The discovery image, shown above , was taken in 2008 but confirmed only recently by noting that the planet stayed with its parent star as background stars slightly shifted over time. ... About APOD | ...

Clues to the formation and evolution of our Galaxy, the Milky Way, are hidden in the chemical abundances and kinematics of its stars. ... The discovery of the ongoing accretion of the Sagittarius dwarf galaxy confirmed that mergers with satellite dwarf galaxies have contributed to the formation of the Galactic halo. ... In particular, I investigated the accretion of dwarf galaxies by the Galaxy and the role of asymptotic giant branch (AGB) stars in the chemical evolution of these systems. ...

... Contacts . 2012: . ... We refined the fundamental parameters of the components, the orbital periods, and the conditions of photospheric heating of the secondary component by the ultraviolet radiation of the hot component. ... The observations of the star clusters associated with ultra-luminous x-ray sources (ULXs) in four galaxies on the 6-meter and VLT telescopes have shown that all the ULXs are located within 200pc of very young star clusters (younger than 5 million years). ... Archive . ...

Next: Low-Mass Star Formation Up: M.D. Smith Previous: M.D. Smith Contents . Massive stars are of elevated importance in our Universe for several reasons. ... During their lives, they influence the nurseries in which new stars might form. ... He and Michael Smith investigated the consequences of massive star formation in one such region of our Galaxy. They uncovered that massive stars are forming in the Rosette Molecular Complex at a rate way beyond previous expectations. ...

... We have assumed a constant in time star formation rate and the total number of stars in the Galaxy, , to be such that the total mass of the galaxy is ; assuming the Salpeter mass function ? , we get . ... This number agrees with a standard estimation of the galactic star formation rate of order of per year. In each run of calculations, we trace the evolution of binaries with initial parameters randomly distributed according to the chosen initial laws. ...

... Posts tagged ?star formation? ... Star Formation via the Little Guy: A Bayesian Study of Ultracool Dwarf Imaging Surveys for Companions by P. R. Allen. ... ArXiv] Bayesian Star Formation Study, July 13, 2007? ... Algorithms arXiv Astro Bad AstroStat Bayesian CHASC Cross-Cultural Data Processing Fitting Frequentist Galaxies gamma-ray High-Energy Imaging Jargon Job Languages MC MCMC Meta Methods Misc News Nuggets Objects Optical Physics Quotes Spectral Stars Stat Timing Uncertainty X-ray . ...

... Science . ... Science Users Information > Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: High-mass Star Formation at High-Angular Resolution . ... Data Handling and Products . ... Science Data Products Forum . ... ESO Data . ... ESO Data Access Policy . ... This project aims to obtain a better understanding of high-mass star formation by performing a comparative study of sites of high-mass star formation that display SiO maser (radio laser) emission. ...

New polar ring galaxies catalogue. ... A host galaxy like S0 or E, the polar component is like spirals or irregular galaxies ( gas -rich and bluer) Not only narrow annuli, but also extended disc-like rings Warped and inclined rings Only 20 large-scale polar rings + 6 inner rings were kinematically confirmed from the Whitmore et al. list: - HI maps (Cox et al; Sparke et al. ) - optical-long slit spectroscopy (Reshetnikov et al) - optical ...

... The Russian TESIS/ CORONAS-PHOTON Solar Observatory, which has been working in orbit since January 30th, 2009, has photographed one of the most important events in the build up to the upcoming solar cycle - the formation of our star's new southern belt of activity. The first magnetic fields of the new cycle in the southern hemisphere appeared on the Sun's surface on May 23-24th. ... The belt of activity is one of the primary concepts, characterizing the solar cycle. ...

... The star formation rate (SFR) of the current SF episode can be estimated from the total H luminosity. ... For the derived total flux F (H )=5.8 erg s -1 cm -2 we obtain a total H luminosity of 10 39 erg s -1 . ... The total mass of ionized gas can be obtained from the average mass density inside the H II region and its volume. An average mass density corresponding to the average electron density of 1 cm -3 within a volume with a diameter of 0.5 kpc yields a total ionized gas mass of 10 6 . ...

... Ciel Espace, le magazine qui vous guide toujours plus loin . ... Ciel Espace, nouvelle formule, c'est . des actualit?йs . ... des pages consacr?йes ?а la publication de vos photos Mais c'est aussi une vraie communaut?й avec laquelle partager votre passion et nourrir votre curiosit?й. Accueil Le myst?иre de la formation des naines brunes enfin r?йsolu ? ... Oph B-11, la premi?иre pr?й-naine brune jamais observ?йe, se forme d'une mani?иre similaire aux ?йtoiles ?а partir d'une condensation de nuage. ...

... Le R?seau de formation et de recherche franco-russe en Sciences et Technologies de l?Information et de la Communication est un Groupement de Recherche International dont la convention de cr?ation a ?t? sign?e en d?cembre 2007 ? ... Moscou par le CNRS et l? INRIA du cot? fran?ais, et par Acad?mie des Sciences de Russie , la Fondation Russe pour la Recherche Fondamentale et Universit? ... La convention est conclue pour une dur?e de quatre ans, ? ... Le r?seau cherche ? ... A ces fins le r?seau cherche...

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