... High-pressures experiments are mostly aimed at studying phase transformations in solids, synthesising new phases and studying their composition, crystal and magnetic structure, physical and thermodynamical properties. ... The specific feature of investigations at LHPP that distinguishes it from most other high-pressure laboratories is combining in situ measurements with studies at ambient pressure of new high-pressure phases fixed by quenching to liquid nitrogen temperature. ...

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... Star formation requires interstellar clouds that are cold and dense enough for self-gravity to overcome internal pressure from gas thermal motions and other factors, thus leading to cloud contraction and eventual collapse to stellar densities. ... Absorption has all of these parameters plus one more describing the fraction of the emission (p) that is behind the absorbing cloud. ... Obser ving Interstellar Hydrogen Clouds Clouds in the ISM can produce either emission or absorption spectra. ...

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... The properties of the dust grains (e.g., temperature and mass) can be derived from fitting far-IR SEDs (т??100 ЮМm). Only with SPIRE on Herschel has it been possible to get high spatial resolution at 200 to 500 ЮМm that is beyond the peak (~160 ЮМm) of dust emission in most galaxies. Aims: We investigate the differences in the fitted dust temperatures and masses determined using only 200 ЮМm data is for deriving these dust properties. ...

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• Spitzer Analysis of H II Region Complexes in the Magellanic Clouds: Determining
• The Herschel revolution: Unveiling the morphology of the high-mass
• Fine Guidance Sensor Instrument Handbook

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• Conservation of Momentum
• THE HUBBLE LAW JAVA APPLET
• Inflationary Epoch

... 2014: . Discovery of two isolated lethargic dwarf galaxies in the Local Group neighborhood . We determined the distances for two dwarf galaxies, KK258 (M B =-10.3) and KKs3 (M B =-10.8), as 2.23 and 2.12Mpc, respectively, with an accuracy better than 4%. ... Catalogue of extragalactic distances . We have compiled a catalogue of estimates of extragalactic distances to galaxies, obtained independently of the redshift. ... The catalogue of extragalactic distances 2014, A , 570, A13 . ...

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• Metagalaxy sector, archive 2013
• topic_en
• IRAS01005+7910

... A consistent theory of turbulence has not been constructed as yet (this problem is linked with one of the one million dollar problems of the Clay Mathematics Institute), and therefore researchers all over the world rely on computer simulations to understand the underlying physics and processes in star forming environments. As computer power grows our simulations become more and more realistic, allowing us to include a lot of interesting and potentially vital physics into our models.  ...

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• Low-Mass Star Formation
• V652HER AND MERGED BINARY WHITE DWARF MODELS
• Armagh Observatory

Next: Determining Gains and Bandpass Up: Calibration, the ATCA, and Previous: Calibration of Data with . ... mfcal : This determines antenna gains, band passes and delays given a point-source calibrator. ... The polarisation properties of the calibrator can be determined as part of the solution process. ... Next: Determining Gains and Bandpass Up: Calibration, the ATCA, and Previous: Calibration of Data with Miriad manager . ...

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• Atmospheric opacity and system temperature
• Research - The high-velocity clouds of M31
• mfcal

Blackholes2 Forum Message . ... Holostars: Black Holes Without Event Horizons . ... Its name derives from the fact tht information is preserved in such a black hole, and must be a contraction of hologram and star. ... The exterior metrics and fields of the charged holostar are equal to the Reissner-Nordstroem black hole solution. ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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... Determining the nominal roll angle for stable intervals . ... We found the necessary information in a file 'rh*.ao', which has a binary extension table for each obi. ... Unlike the question of determining the nominal roll angle, we know of no a priori indication of this problem (although the guide star configuration may be the cause, or at least associated with this condition): it is necessary to examine the source position for each obi. ... The guide star record is at the end of the 'anc file'. ...

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• Microcalorimeters
• Very Low Mass PMS Objects

... When creating a mosaic from a set of individual frames, the correct background offset for each frame must be determined for proper matching. In this paper we describe a method for constructing a mosaic from a set of individual frames by applying a minimization technique. ... Typically these are frames with some known defect (see ? ... Determining which frames to exclude from the final mosaic is critical, since one bad frame can create background offset errors that propagate throughout the mosaic. ...

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• A Technique for Determining Proper Motions from Schmidt Plate Scans at ST ScI
• Determination of the Permissible Solutions Area by Image Reconstruction from a
• ADASS 2003 Conference Proceedings

... Development of Ideas of Structure and Evolution of Stars. Integral Features of Stars, Which Determine Their Structure, Direction and Rate of Evolutuion. ... Connection between Potential and Thermal Energy of Star. ... Structure of a Main Sequence Star. Features of Massive Stars Evolution on the Main Sequence. Internal Structure of the Sun. ... White Dwarfs, Their Features. ... Evolution from the Main Sequence of Massive Stars. ... Evolution of Small Mass Stars till White Dwarfs Sequence. ...

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• Theoretical Astrophysics

Physica C 1 PHYSICA C C ELSEVIER CONDUCTIVITY and Antiferromagnetism of CaCuO2 Thin Films Doped by Sr Gennady A. Ovsyannikova,b*, Viktor V. Demidovb, Yuli V. Kislinskib, Philippe V. Komissinskia,b, Dag Winklera a Chalmers ... revised date here; accepted date here Abstract The results of electrical and magnetic investigations of epitaxial CaxSr1-xCuO2 ( CSCO ) thin films grown by pulsed laser deposition are presented ... Temperature dependence EPR amplitude for two CSCO films with =0.15 ...

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• http://www.cplire.ru/nano/publications/JETP105-235.pdf
• Magnetic field influence on martesite phase transition in Ni2+УMn1-УGa
• Project 4 - RFBR - Stepantsov, Determination of the space anisotropy of order

... Orion Star Colours . ... Red stars are cool, around 3,000 kelvins (K), while blue stars are hotter and can have temperatures over 30,000 K. Our own lovely yellow Sun's temperature is a comforting 6,000 K. Hydrogen Trifid . ... Clouds of glowing hydrogen gas mingle with dark dust lanes in the Trifid Nebula, a star forming region in the constellation Sagittarius. ... These are galaxies of the Hercules Cluster, an archipelago of "island universes" a mere 650 million light-years distant. ... Vega . ...

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THE CHEMICAL COMPOSITION OF REGOLITH AT THE MOON'S SOUTH POLE, ACCORDING TO DATA OF LUNAR PROSPECTOR AND LUNAR RECONNAISSANCE ORBITER MISSIONS. ... Introduction: The article tells about the results of integrated study of the craters at the Moon's South Pole with permanently shadowed region of craters. ... We have compared the ultimate composition of the soil matters in the craters with "cold traps" in the Moon's South Pole with regard to thorium, ferric oxide and hydrogen contents (Fig. ...

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• http://selena.sai.msu.ru/Chik/Publications/Aitken/MS015.pdf
• http://selena.sai.msu.ru/Shev/Publications/m44_76_sinitsin_shevchenko.pdf
• http://selena.sai.msu.ru/Pug/Publications/ms34/MS058.pdf

Next: WWW access Up: No Title Previous: Initial parameters of compact . The World Wide Web version provides the opportunity to construct an evolutionary track with all important parameters determined by the user at will from a broad range of available values. Figure: Part of the table for the defauly output. Some of the most unclear branches of the scenario can also be determined by the user. ... Figure: Graphical diagram for the default output . WWW access . ...

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• No Title
• Case B: #tex2html_wrap_inline768#
• Introduction

... The formation of spectral disturbances of Cosmic Background Radiation (CBR) during the period of hydrogen recombination at redshift is considered. Special attention is paid to the decimeter and meter wavelength band. ... In this paper we will return to the question on the spectral lines caused by recombination of hydrogen discussed by Dubrovich (1975) , in the longer wavelength part of spectrum of the CBR. ... A synthesis of recombination radiolines spectra is divided into several stages. ...

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• Astrophysics Group CosmoNet
• Research
• High resolution studies of protostellar condensations in NGC 2024

Our group is involved in theoretical and observational research in several topics of star formation. ... The Arcetri group is carrying a coordinated effort to determine the kinematics and physical parameters of clouds where high-mass stars form. Massive stars form in association with solar mass objects from gas clouds of mass anywhere between one hundred and ten thousand times that of the sun. ... Disks around young stars: Inferring planet formation . ... Star Formation Group Page . ...

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• CHIANTI atomic database
• The Arcetri Spectral Code file format
• research field

XMM-Newton Science Analysis System Page: 1 orbit June 28, 2006 Abstract Create a FITS timeseries \HK-like" le from the ODF Spacecraft Reconstructed Orbit File. ... Both sets of values will be written into a standard OGIP-compliant FITS binary extension table with a TIME column value, derived from a start, stop and sampling interval time, each speci ed by the user. ... StartANDEndNotInODFRange (error) Start AND End times selected not congruent with input ODF obs times. ... SAS ODF must be properly set. ...

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• http://xmm.vilspa.esa.es/sas/8.0.0/doc/orbit.ps.gz
• http://xmm.vilspa.esa.es/sas/5.4.1/doc/orbit.ps.gz
• http://xmm.vilspa.esa.es/sas/6.5.0/doc/orbit.ps.gz

There are many ordinary/partial differential equations/systems describing various phenomena in physics, mechanics, chemistry, biology, sociology, etc. ... Prerequisites: 1 semester "Advanced Calculus", 1 semester "Linear Algebra". Optional: 2 semester "Advanced Calculus", 2 semester "Linear Algebra", 1 semester "Functions of Complex Variables", elements of the functional analysis and the ordinary differential equations theory. ... Laplace transform for linear differential equations . ...

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• Conf rence "Zeta Functions"

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

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• Результаты научных работ 25
• Results scientific researchs 19
• Laboratory of spectroscopy and photometry of extragalactic objects : Vortex1