ChASeM33 . The Chandra ACIS Survey of M33 - . ... The major sources of feedback into the ISM are massive OB stars, which inject energy via Lyman continuum photons, stellar winds and, finally, supernova explosions. ... SB interiors are generally more efficient than individual SNRs in converting thermal into kinetic energy of expansion, because radiative losses are smaller in SBs than for the same number of isolated explosions. ... 1) Is the diffuse hot ISM shaped predominantly by SNRs or by SBs? ...

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• Vertical Structure of the Secondary: Hydrostatic Model
• Home Page for SAOimage: The Next Generation
• The Chandra Multiwavelength Project (ChaMP)

Chiaki Kobayashi, Ralph Sutherland How galaxies did form and evolution? - to answer this unsolved problem, we are simulating the formation and evolutionary history of galaxies in the Universe, including star formation, supernovae feedback, and chemical enrichment. Comparing the spacial distribution of elements within galaxies with observations, we will examine fundamental physical processes that drive galaxy formation. ... COALA : Universe Galaxy AGN Star Planet ...

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• GSAOI Bulk Motions Science Page
• Philip Lah's Research
• Naomi McClure-Grffiths

Next: Implementing a New Data Archive Paradigm to Face HST Increased Data Flow . ... There have been two generations of archive systems (DMF and DADS) and user interfaces (STARCAT and StarView). In this paper, we describe recent projects and future directions in the continued evolution of the HST Archive. ... StarView is supported in CRT and X/Motif modes on Sun and Digital platforms. ... We continue to improve the HST Archive systems-DADS, StarView, and the new Web interface. ...

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• Projective Transform Techniques to Reconstruct the 3-D Structure and the
• Design and Implementation of CIA, the ISOCAM Interactive Analysis System
• Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron

... The study of the Large-scale structure of the Universe and measurements of the Dark Energy equation of state; The exploration of the growth and cosmological evolution of supermassive Black holes in the Universe. ... In course of the all sky survey SRG will discover about 100 000 galaxy clusters and 3 million AGNs. Galaxy clusters are the largest gravitationally bounded objects in the Universe and are best explored through the study of X-ray emission from the hot intergalactic gas. ... 2016 IKI RAN ...

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• z90-program
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• Second Spectrum-RG/eROSITA Conference

... We consider the astrophysical evolution of the Galaxy over large time scales, from early stages (an age of ~10 8 yrs) to the end of traditional stellar evolution (~10 11 yrs). ... In the model considered, the basic stages of Galactic evolution are as follows. ... Essentially all other basic parameters of the Galaxy vary little. ... The final "stellar epoch" in the life of the Galaxy is completed ~10 13 yrs after its formation, when the evolution of the least massive stars comes to an end. ...

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• Home page of Dmitri Wiebe
• Publications of Dmitri Wiebe
• Основные публикации Дмитрия Вибе

Next: General CCF Components Up: Calibration Access and Data Previous: List of CAL Routines Contents . This section contains descriptions of the structure of CCF constituents. ... The calibration team of the SOC is also providing additional CCF components where required in conjunction with data that were generated with SciSim. ... These CCF components are generated on a need basis and are identical in structure to the real life components. ... Generation from Ground Calibration Data . ...

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• OM Related CCF Components
• Errors
• Input Files

... Ultracold Big Bang experiment simulates evolution of early universe . ... Professor Cheng Chin and his University of Chicago associates have simulated the impossibly hot conditions that followed the Big Bang within an ultracold vacuum chamber in his sub-basement laboratory in the Gordon Center for Integrative Science. ... This is the first time an experiment like this has simulated the evolution of structure in the early universe, said Cheng Chin, a professor at the University of Chicago. ...

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• How do neutron stars generate steady magnetic fields? | Astronomy.com
• Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets,
• Cosmic evolution in a computer | Astronomy.com

Solar Flare Origin - critical analysis" Lev Pusti'lnik We analyze current approach to solar flare origin in 3 aspects: a. Pre-flare equilibrium state of current-magnetic structure above active region and its evolution to flare state, b. Possible reasons of stability loss with transition of system in flare state c. Flare energy release in turbulent current sheet and particle acceleration in this system. ...

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• AGB and Post-AGB Evolution: Structural and Chemical Changes
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Physics and
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Magnetic stars -

... the radiative transfer equation (RTE) for the randomly-irregular magnetized plasma has been derived on the base of general grounds of the multiple scattering theory . ... Solutions of several absolute tasks of the scattering theory have been obtained (on the optical depth of the ionospheric plasma layer, on the value of radio wave anomalous attenuation, on anomalous refraction, on the backscattered signal intensity for the source being placed within a plasma layer). ...

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• Vladimir Marsakov Publication List
• Vladimir Marsakov Abstracts
• Zabotin Nikolay