... А.М. Белобородов (Колумбийский университет, США) . ... Рабочий язык конференции - русский. ... Е.М.Чуразов, д.ф .- м.н . А.А. Вихлинин, проф. д.ф .- м.н . М.Р.Гильфанов, д.ф .- м.н . М.Н.Павлинский, д.ф .- м.н . М.Г.Ревнивцев, д.ф .- м.н . С.Ю.Сазонов. д.ф .- м.н . М.Н.Павлинский (председатель), к.ф .- м.н . А.В.Мещеряков (зам. председателя), Н.Л.Александрович, к.ф .- м.н . В.А.Арефьев, к.ф .- м.н . Р.А.Буренин, П.Болдин, Н.П.Васильева, к.ф .- м.н . А.А.Воеводкин, В.Воробьев, А.Е.Елкин, ...

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. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

... CfA Home . HCO Home . SAO Home . ... Welcome to CfA . CfA History . ... Laboratory Astrophysics . Extreme Astrophysics . ... 617) 495-7210 . ... 617) 495-7044 . ... 617) 495-7265 . ... HEA Research . ... HEA Home Page . CFA/HEA Home Page . ... High Energy Astrophysics Division (HEAD) . Chandra X-ray Center . ... Chandra Cluster Cosmology Project . Chandra Multiwavelength Project (ChaMP) . ... Chandra-Planck Clusters Project . ... CfA Virtual Observatory Project . ...

February 5, 2001 (Monday) Jim Brau, UO Center for High Energy Physics . February 19, 2001 (Monday) Shane Larson, Montana State University . March 5, 2001 (Monday) Xiao-Gang He, National Taiwan University . return to top . 4:00pm, 318 Willamette Hall . ... I will also discuss ways to determine the CKM unitarity triangle and new physics beyond the Standard Model using various B decays. 4:00pm, 318 Willamette Hall . ...

... The research activity of the Group is mainly on the theoretical side, although our work plays an important role in the planning of scientific objectives of experiments and telescopes aimed at investigating the high energy universe, as well as being used to interpret the wealth of data that shed light on the violent universe from Earth and from Space. ... This email address is being protected from spambots. You need JavaScript enabled to view it. ...

The approaches mentioned in the section title belong to one family which is called in Newton's book [ 56 ] the short waves or high energy approximation (HEA). It means the scattering by soft particles (or potentials) in the case of the wavelengths short in comparison with the particle size (or correspondingly the case of scattering of high energy particles by the potentials). ...

... A High Energy Fleet . ... 24.05.1998 . ... Courtesy: MSFC Historical Archive , NASA Explanation: Looking like a fleet of futuristic starcruisers, NASA's highly successful series of High Energy Astrophysical Observatory (HEAO) spacecraft appear poised over planet Earth . ... HEAO-1 and HEAO-2 were responsible for revealing to earthlings the wonders of the x-ray sky , discovering 1,000s of celestial sources of high-energy radiation. ... 2007 2008 . ... Publications with keywords: satellite - X-ray . ...

... May 24, 1998 . A High Energy Fleet . Courtesy: MSFC Historical Archive , NASA . Explanation: Looking like a fleet of futuristic starcruisers, NASA's highly successful series of High Energy Astrophysical Observatory (HEAO) spacecraft appear poised over planet Earth . Labeled A, B, and C in this vintage illustration, the spacebased telescopes were known as HEAO-1 , HEAO-2 , and HEAO-3 respectively. ... Archive | ... About APOD > . ... NASA Technical Rep.: ...

Next: The interstellar medium Up: An overview Previous: Radio pulse characteristics . Mostly the very youngest pulsars . Just 3 pulsars detected at Optical Wavelengths . Crab, Vela, B0540-69 . X-ray - 27 detected, 13 pulsed . Gamma ray - 6 detected all pulsed . Radio emission of spin down energy . ... Need radio ephemeris . 18000 pulse periods elapse between each EGRET photon detected from the Crab pulsar . ...

To obtain more information about satellites observing the sky in x-rays and gamma rays, you can contact the archive of the Laboratory for High Energy Astrophysics at Goddard Space Flight Center. Some documents in that archive can be linked directly from here: . General Information . ... Small Astronomy Satellite 3, a follow-up mission. HEAO 1 , High Energy Astronomical Observatory 1. ... Exploration" home page (index) Glossary . Official GSFC Home Page .. NASA WWW Home Page . ...

... Geoffrey Bicknell . Following are my lecture notes more or less in the order that I give them, together with exercises and relevant papers and images. ... Lectures and tutorial Monday 09:30 Lecture - Duffield Lecture Theatre . Tuesday 11:00 Lecture - Duffield Lecture Theatre . Wednesday 09:30 Lecture - Duffield Lecture Theatre . ... Lecture notes: . Overview of High Energy Astrophysics . ... Questions 1-4; due 27 Feb . Questions 5-8; due 6 March . ... Figure 1 for above paper . ...

... Samara region . SSAU History . SSAU roadmap . ... International relations . Scientific Publications . ... What You Should Bring Along . ... Events The International Youth Scientific School 'Materials science and high-energy processing' . Russia, Samara, SSAU . Event type: Youth Scientific School . ... The International Youth Scientific School 'Materials science and high-energy processing' will take place in SSAU from 14 to 22 September 2015 in SSAU of Samara city. ...

... The second catalog of high-energy gamma-ray observations from the Energetic Gamma Ray Experiment Telescope (EGRET) on the Compton Gamma Ray Observatory includes data from Phase 1 (1991 April - 1992 November) and Phase 2 (1992 November - 1993 September) of the mission. ... Also included are approximate upper limits for gamma-ray sources at any point in the sky and information about sources listed in the first EGRET catalog but not appearing in this one. gamma rays: general . ... Source Detections . ...

... If requested ( runbackground =Y), the task creates a background lightcurve, as well as a background spectrum for the imaging modes (FF, eFF, LW, SW) using background masks. ... The background masks are created by task badpixfind using threshold parameters, appropriate for the detection of real X-ray sources. ... As the GTIs strongly depend on the intended science this screening is not performed and only background masks, the lightcurve, and a GTI file are created by epchain . ...

Next: Optical Jets in Up: QSOsGalaxies, and Previous: Quasar Spectral Features . ... High luminosity and high redshift combine in quasars to give conditions that allow studies of the intergalactic medium, as well as the emission mechanism in quasars. ... We present results of the modeling of the spectrum of the high redshift ( z =2.72), high luminosity ( 10 ergs s ) quasar, HS1700+6416 (Reimers et al. 1989), observed with HST FOS (Reimers et al. 1992) and GHRS (Reimers 1995). ... 1995). ...

... 01.04.07 - CONDENSED MATTER PHYSICS . HIGHER CERTIFICATION COMMITTEE . MINIMUM PROGRAM . ... 01.04.07 тАУ Condensed Matter Physics . ... The program is based on the principle divisions of Condensed Matter Physics. ... Types of bonding force in condensed matter: Van der Waals bond, ionic bond, covalent bond, metallic bond. ... Structure of matter with unidirectional interaction. ... Covalent bond structure of matter. ... Diffraction on amorphous matter. ... High temperature superconductors. ...

Next: The ``Reflection'' Effect Up: Ejectors in Massive Binary Previous: The Radiopulsar PSRB1259-63 - a . The radiopulsar PSRB1259-63 in a massive binary has an extremely high eccentricity (Johnston et al. ... We have assumed that explosion occurs at a random moment on the orbit and all the mass thrown off by a star instantly leaves the system because the characteristic velocity of matter from the exploded star is much higher than the orbital velocity. ...