... Modern problems of physics and dynamics of the solar system". Kyiv, October, 4-10, 2000. 2001. ... 2000. ... Криводубський В.Н., Крячко ?. ... Evtushevsky O.V., Milinevsky G.P., Kravchenko V.O., Gritsai Z.I "The high-speed initial expansion of the barium atoms and ions in the CRRES Caribbean releases" // В?сник Ки?вського ун-ту. ... Tugay A. "Galaxy distances data unification from RFGC and Mark-3 catalogues" // 8th Open Young Scientist' Conference on Astronomy and Space Physics. ...

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• Косм?чний експеримент
• CAMERA ELECTRONICS FOR THE CCD FOURIER SPECTROMETER

Next: Calling Parameters Up: CAL_getRedistribution Previous: CAL_getRedistribution Contents . The redistribution function of the CCD's is parameterized per CCD and per node. ... It combines the X-ray absorption probability in silicon with an empirical parameterization of the generated charge signal, which is then folded by a Gaussian for noise representation. ... For a given photon of energy (in eV), and absorption at , the collected charge (in eV) is parameterized with the empirical model . ...

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• Front Illumination
• Deep Depletion
• Energy resolution

What happens to a star heavier than five solar masses? ... Stars about ten solar masses probably behave like our five solar mass star until they reach the end of core-helium burning. ... The Crab nebula was formed after a massive explosion ripped a star apart in 1054. ... Today, the glowing outer layers of the star are still rushing away from a tiny star in the centre. ... An incredible explosion rips through the outer layers of the star, releasing colossal amounts of energy in a supernova explosion. ...

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• M.D. Smith, Research Astronomer
• Atomic data for Stellar Atmospheres: lte_lines
• NeditPage1

... SEARCH ASP SITE: Match ALL words Match ANY word . Programs . ... Galileo Teacher Training Program . Galileo Educator Network . ... Family ASTRO Discover a new program at the ASP that is developing events and activities to share the excitement of hands-on astronomy with families . ... The Survey of College Astronomy Teachers Add your voice to a growing network of educators who teach introductory astronomy at community colleges and other institutions without extensive research programs . ...

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• ASP: Sharing the Universe
• ASP: IYA 2009
• ASP: Survey

Some recent results ( see ) attracted the attentions of astronomers working on field which could benefits from photon counting techniques with high speed and spatial resolutions as adaptive optics. ... Fasti has been designed to be fast and largerly configurable. ... The data rate attined in the best case (30 Mhz), give no impossible load to the digital acquisition in the photon counting mode, since data are 1 bit only, they can be parallelized, giving a maximum speed of about 940.000 32 bit word/sec. ...

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• Arcetri Star-Formation Group Publications
• Observing capabilities
• Roba Simone Busoni

... We have performed a series of tests to find an optimal data distribution in the Cray T3D memory, and to identify a strategy for the Dynamic Load Balance (DLB). ... N-body simulations are one of the most important tools in contemporary theoretical cosmology, however the number of particles required to reach a significant mass resolution is more larger than those allowed even by present-day state-of-the-art massively parallel (Gouhing 1995; Romeel 1997 & Salmon 1997) supercomputers (hereafter MPP). ...

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• Preface
• The AXAF Science Center Performance Prediction and Calibration Simulator
• News on the ISOPHOT Interactive Analysis PIA

Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Space Flight . ... Some 13.7 billion years ago, a mere millionth of a second after the Big Bang, the first hydrogen and helium nuclei condensed out of a hot, dense soup of quarks and gluons. ... In the very last few kilometres some of the light was scattered by a myriad of water droplets (containing hydrogen nuclei which had existed almost since the Big Bang) slowly descending through the air following a rainshower. ...

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• COROT-7b: Exoplanet with a sky made of stone | Astronotes
• Kepler-10c: the First Mega-Earth | Astronotes
• Pseudoscientific ideas so bad that they're not even wrong | Astronotes

CFITSIO Interface Library CFITSIO is a library of ANSI C routines for reading and writing FITS format data files. ... The CFITSIO library is built on Unix systems by typing: > ./configure [--prefix=/target/installation/path] > make (or 'make shared') > make install (this step is optional) at the operating system prompt. The configure command customizes the Makefile for the particular system, then the `make' command compiles the source files and builds the library. ...

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... Bad Astronomy . ... Bitesize Astronomy . ... even the brightest star won't last forever.' ... The pressure and heat are so enormous inside the star's core that hydrogen is fused into helium. ... A star like the Sun has enough hydrogen to keep its fusion fires going for billions of years, but a star like Rigel, a massive star in Orion, burns its hydrogen so fast it may run out in just a few million years. ... The problem is, at this point something bad happens: silicon fuses to iron. ...

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• Phil Plait's Bad Astronomy: Phil's Los Angeles Adventure

... 1 - 5 m HgCdTe Detector Material . Hybridization of 2048 x 2048 Arrays . ... Options for Extension to Visible Wavelengths . ... MBE HgCdTe Capability at Rockwell Science Center . ... Over the last two decades, dramatic improvements in the performance of 1 - 5 m infrared detector materials combined with the leap from single detectors to million pixel arrays have led to a billion-fold improvement in our ability to observe astronomical sources at these wavelengths. ...

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... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... On-Line Proposal Applications and Links (OPAL) . ... Parkes | ... Astronomical tools & software . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Photometry Theory . ... Colour Indices provides details and values for colour indices for different spectral and luminosity classes of stars...

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• first_mm_light
• TWENTY-FIVE YEARS OF AUSTRALIAN IR
• Yiannis Web Page

HARP is the Heterodyne Array Receiver Programme for the James Clerk Maxwell Telescope. The programme is beginning with HARP-B, . ... February 2006 . ... The HARP-B project is a collaboration between Cavendish Astrophysics (MRAO) at the University of Cambridge, UK, The Joint Astronomy Centre at Hilo in Hawaii (operators of the JCMT), The UK Astronomy Technology Centre at the Royal Observatory Edinburgh, The Herzberg Institute of Astrophysics of the National Research Council Canada . ...

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• Finder Documentation

... NVIDIA, the NVIDIA logo, NVIDIA nForce, GeForce, NVIDIA Quadro, Vanta, TNT2, TNT, RIVA, RIVA TNT, Quincunx Antialiasing, and TwinView are registered trademarks or trademarks of NVIDIA Corporation in the United States and/or other countries. Linux is a registered trademark of Linus Torvalds. ... OpenGL is a registered trademark of Silicon Graphics Inc. ... Installing the NVIDIA Driver . ... Configuring X for the NVIDIA Driver . Using nvidia-xconfig to configure the X server . ...

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• vertex drive system
• AOFTM Help Page

Supernovae are simply stars which explode. ... To understand supernovae, we need to understand stars. ... In this stage our Sun will swell up hundreds of times its current size, swallowing the Earth, and glowing hundreds of times brighter than it is now. ... Stars more than 10 times the mass of our sun have much more exciting lives. ... A Type II supernova to be precise. ... Since 1995 two teams have been discovering these objects: Our team, the High-Z SN Search, and the Supernova Cosmology Project. ...

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