An Ancient Universe: How Astronomers Know the Vast Scale of Cosmic Time . THE PROCESS OF SCIENCE: HOW DO WE KNOW? The nature of the universe, its age, its birth and life story, have been deduced through the process of science. ... In the case of astronomy, it usually starts with making careful observations and measurements -- something your students can begin to do through inspection of astronomical images, and observation of the real sky. ... An Ancient Universe - Table of Contents . ...

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• ASP: Editorial
• ASP: An Ancient Universe - The Age of the Oldest Stars
• ASP: A High School Curriculum in Astrobiology

... Study of Mg-Fe-silicate glasses of variable composition. ... With the new data, the astrophysical discussion started in Paper I was continued and focussed on the comparison of the olivine glass data with IRAS LRS spectra of O-rich circumstellar envelopes around Mira stars. ... The new olivine glasses point to the interesting consequence that the temperature for silicate dust grains at the inner edge of circumstellar envelopes must be considerably higher than the values often given in the literature....

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• Optical constant database - Level: measurement/paper
• Radiation mechanisms of astrophysical objects: classics today | Механизмы
• Processes

I was born in 1955, finished well-known 2nd school (mathematical) in Moscow, graduated at mathematical department of Moscow State University (MSU). My current positions are sci. researcher at Institute of Mechanics MSU and Network admin at Sternberg Astronomical Institute MSU. ... Hobbies: Anchient history, swimming, yachts, drinking vodka and good vine. ... Rambler in Russia: Some notes (in russian). ... For AstroNet users: see Netiquette in AstroNet (in Russian) for our administrative policy. ...

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• SN 1989B Light Curve Analysis.
• Zen: q3c adass abstract
• Further Information and Bibliography

The revision of the MASS/DIMM star catalogue N. Shatsky, V. Kornilov March 16, 2008 Abstract The compilation of the (updated) version of the MASS (MASS/DIMM) device target catalogue is described. ... Then the list was cleaned according to following criteria: I. Remove stars too faint for a MASS device. ... Here the color equation of the Sternb erg device was taken: M AS S mag = V mag + 0.45 (B - V ); stars with M AS S mag > 3.2 were removed. ... This was made based on the GCVS4.2 catalogue data. ...

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... Because of the low conductivity, the magnetic coupling is weak and depends critically on density, temperature, ionisation rate and charged species. ... Implications When the Hall regime dominates near the midplane and ambipolar diffusion is dominant closer to the surface, a thicker layer of the disc is unstable to MRI perturbations and modes grow faster than under the ambipolar diffusion approximation. ... Right panel: For weak coupling, Hall limit perturbations grow until vA/cs ~ 2.9. ...

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• Marc White - Astrophysicist - The Australian National University
• Raquel Salmeron - Research Interests and Experience
• Mike Bessell, MSSSO - Images

... Dept. for Physics of Planetary Systems . ... Laser station . ... Built a network of laser stations (LLS), radio (GNSS) satellites and observation radiointerferometrychnyh observations of quasars (VLBI) ( YA.S. Yatskiv, Medvedsky MM, AA Pace, EE Volvach, YL Kokurin in collaboration with workers in other entities) . ... БЂў Laser station observation satellites is the global network of service stations of the International Earth rotation and conducts active surveillance for international programs. ...

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• КАРТОТЕКА ПУБЛ?КАЦ?Й СП?ВРОБ?ТНИК?В ГАО НАН УКРА?НИ
• Area of scientific investigations
• Dept. for Astrometry & Space Geodynamics

... Telescopes . ... 1995: . ... This sample proved to be the deepest one of all the analogous samples by the highest redshift estimates. ... More than 70% of dwarf galaxies from the sample were resolved into stars. ... Based on the results of optical and radio observations of a sample of 100 blue dwarf compact galaxies with the telescopes in the SAO RAS, France and USA the estimates of a total dynamic mass and the ratio of dark halo mass to the mass of the whole luminous matter were obtained. ...

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• Galaxy sector, archive 2012
• Detection of Radio Transients and Variable Radio Sources Using the Archive Data
• Electronic version of Russian Bulletin

SOLAR POLARIZATION 5 ASP Conference Series, Vol. 405, c 2009 S. V. Berdyugina, K. N. Nagendra, and R. Ramel li, eds. Fine-scale Sto chastic Structure of Solar Magnetic Fields V. Chertoprud, B. Ioshpa, and V. Obridko Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences, Troitsk, Moscow Region, 142190 Russia Abstract. ... The exponent H is 0.5­0.7 for the active region magnetic fields and 0.1 for the background field. ...

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• http://www.izmiran.rssi.ru/~sova/Copies/asr00-26-1219.pdf
• http://www.izmiran.rssi.ru/~obridko/papers/320.pdf
• http://www.izmiran.rssi.ru/~obridko/papers/360.pdf

Альтернативный форум . Scientific.ru Все форумы . ... Отмечать NEW , ! ... ETHER SPACE-TIME & COSMOLOGY . ... Volume1: Modern ether concepts relativity and geometry . ... First, there was the evolution of Relativity, Relativistic Cosmology and Geometrodynamics which discarded the early 20th C passive, rigid, ether in favour of geometrized space-time. ... He denominated it 'new ether' because, in opposition to the old one, the new one did not violate his Special and General Principle of Relativity. ...

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• Scientific.ru Общий форум

... We show the analysis of low-hard and intermediate states of sources XTE J1550-564, H 1743-322, GX 339-4, XTE J1859-226, XTE J1650-500 and GRS 1915+105. ... Directly applying the scaling technique we also obtain that a ratio of the BH masses in XTE J1859-226 and in XTE J1550-564 is , and the corresponding ratio for XTE J1650-500 and XTE J1550-564 is . These values of scaling factors r implies that BH masses are ; solar masses in XTE J1859-226 and XTE J1650-500 respectively. ...

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• Истомин Яков Николаевич (ФИАН)
• The 6th INTEGRAL Workshop "The Obscured Universe"

... Space flight . Crew training . ... A task of selection and preflight training is to form up and to train a crew for a space mission. ... Training in crews on the "Soyuz" transport space vehicle and on the "Earth-Moon-Earth" interplanetary flight program, . ... Basic space training of a lunar crew provides for acquiring a fundamental knowledge on the origin, structure and evolution of the Universe, studying methods and means of space flights performance, use of space for the benefit of mankind. ...

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• Project Space Hotel

.

53. SMIS IKI RAN (Sample Images / Miscellaneous)

54. Carrying out of the experiments on the orbital station MIR

55. Server-Wide Configuration

56. Научный отчет ИСЗФ СО РАН по программе Президиума РАН ? 6'Нейтринная физика'

57. Heracles

58. http://www.tesis.lebedev.ru/en/docs/1533.pdf

59. timekeepe

60. Radioastrophysical Observatory ISTP RAS SB