... 1 P. N. Lebedev Physical Institute 1 2013 , 1 Wtot WA 103 - 1-100 104 . B = eB 10 - 1011 , B = mc 10 B = 2Bc = 1 - 10cm = n GJ = Komissarov, MNRAS, 359, 801, (2005) McKinney, Tchekhovskoy, Blandford MNRAS, M 10 - rg = 2GM 1011 - 10 c2 nGJ 10-2 3mc 3 c = 2e2 2 10 6 B , 180, 1241 (2010) Beskin, Kovalev, Nokhrina arXiv:1107.0565 B 2 ce n n lab = Ba 2 er g , c= 1010 M GJ rg 1013- 10 14 a 0.1 15 423, 3083 (2012) , E E E kin kin kin mc 2 - mc 2 - mc 2 - . ...

... X-ray data of GX 3+1 (4U 1744-26) obtained in broad energy ranges using BeppoSAX (0.1­200 keV) and Rossi X-Ray Timing Explorer (RXTE) (3­200 keV) offer a unique The Astrophysical Journal, 747:99 (15pp), 2012 March 10 Seifina & Titarchuk possibility to further investigate, in detail, the evolution of X-ray spectral properties during transition events. ... In Figure 2, we illustrate our spectral model as a basic model for fitting the BeppoSAX and RXTE spectral data for GX 3+1. ... Figure 4. ...

... First Estimate of the Value of the Instrumental Polarization of the RadioAstron Space Radio Telescope Using the Results of an Early Scientific Program for Observing Active Galactic Nuclei I. N. Pashchenko, Yu. ... For this, it is necessary to construct a joint distribution of the observational data and unknown parameters, including both instrumental effects and the parameters of the observed source. ... Unknown parameters. ... Thus, the probability model used is based on the linear model of leakage....

... GOES ACE. ... 103 29 1989 . ... E > 10 (1), > 30 (2), > 60 (3) > 100 (4) 29 1989 . GOES. 29 1989 . GOES, MET), . ... GOES-11, http://sec.noaa.gov/ftpmenu/plots/2005_plots/proton.html ( ) , ( ) . ... Solar Event Reports 2005 http://sec.noaa.gov/ftpmenu/indices/2005_events.html , , 88 , , . ... GOES-11 E > 10, >50 >100 . http://sec.noaa.gov/ftpmenu/lists/particle.html, . ... GOES-11, http://sec.noaa.gov/ftpmenu/lists/pchan.html NGDC http://spidr.ngdc.noaa.gov/spidr ( 3 ) ( 9В15 ). ...

UX Tau A's protoplanetary disk extends to a radius of 120 AU (1 AU = the distance between the Earth and the Sun) with a high spatial resolution of 0.1" (arcsecond) Left: Near-infrared intensity image of UX Tau A. White is the brightest, and then red. ... Its west side (on the right) is a little brighter than its east side; this indicates that the inclination of the disk is in the east-west direction and that its west side is closer to the observer (see figure on the right). ...

... Telescope: TeleVue-85 . ... Integration: 0.1 hours . ... Bortle Dark-Sky Scale: 5.00 . RA center: 83.596 degrees . DEC center: -5.499 degrees . Pixel scale: 1.955 arcsec/pixel . Orientation: 115.687 degrees . Field radius: 1.287 degrees . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

GCVS Variability Types and Distribution Statistics of Designated Variable Stars According to their Types of Variability ======================================================================== I. GCVS Variability Types. ... Amplitudes usually do not exceed 0.1 mag. ... RR Variables of the RR Lyrae type, which are radially-pulsating giant A-F stars having amplitudes from 0.2 to 2 mag in V. Cases of variable light-curve shapes as well as variable periods are known. ... RV Variables of the RV Tauri type. ...

Mon. Not. R. Astron. Soc. 349, 1397­1418 (2004) doi:10.1111/j.1365-2966.2004.07619.x The 2dF QSO Redshift Survey ­ XII. The spectroscopic catalogue and luminosity function S. M. Croom,1 R. J. Smith,2 B. J. Boyle,1 T. Shanks,3 L. Miller,4 P. J. Outram3 and N. S. Loaring4,5 1 2 3 4 5 Anglo-Australian Observatory, PO Box 296, Epping, NSW 1710, Australia Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD Department of Physics, University of

Solar Physics (2006) 233: 89-106 DOI: 10.1007/s11207-006-2850-y C Springer 2006 ON THE POSSIBLE CONNECTION BETWEEN PHOTOSPHERIC 5-MIN OSCILLATION AND SOLAR FLARE MICROWAVE EMISSION A. G. KISLYAKOV and V. V. ZAITSEV Institute of Applied Physics, Nizhny Novgorod, Russia (e-mails: agkis@appl.sci-nnov.ru; za130 Dynamic spectra of low-frequency modulation of microwave emission from solar flares are obtained. ... PHOTOSPHERIC 5-MIN OSCILLATION AND SOLAR FLARE MICROWAVE EMISSION 93 Figure 2. ...

... Рейтинговый каталог астрономических персональных страниц России, версия от . ... Персональные астрономические страницы любителей. ... Астрономический институт Санкт-Петербургского Университета Staff Homepages - здесь собраны сотрудники, имеющие персональные страницы, всего их 12. ... до 10 баллов) . ... 1.0 (первый рейтинговый каталог астроресурсов России - данный текст) . ... Государственный Астрономический Институт им. Штернберга МГУ : SAI Crimean Observatory: 15 человек, персональных страниц -...

... GAM ­ , , GAM ­ . ... 2014 . ... J2000, 90-2. , . ... 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 2 015 015 015 015 015 016 016 016 016 016 017 017 017 017 017 018 018 018 018 018 019 019 019 019 019 /03 /05 /07 /10 /12 /02 /05 /07 /09 /11 /02 /04 /06 /09 /11 /01 /04 /06 /08 /10 /01 /03 /05 /08 /10 /1 /1 /2 /0 /1 /2 /0 /1 /2 ... 18 18 18 18 18 18 18 18 18 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 :17 : 30.000 : 30.000 ...

... Bad Astronomy . ... Bitesize Astronomy . ... Here's a question for you: if you were to place the Moon randomly anywhere in the sky, on average, how many stars would it cover up? ... We found that the sky is about 40,000 square degrees . ... The area of a circle is pi * radius^2, so the Moon's area is pi * (1/4)^2=0.2 square degrees. So the number of stars in an area the size of the Moon is 0.15 stars/square degree * 0.2 square degrees=0.03 stars per Moon area. ... 2008 Phil Plait. ...

... 2003 . ... Astrophysics of isolated neutron stars: radioquiet neutron stars and magnetars Sergei B. Popov; polar@sai.msu.ru; popov@pd.infn.it Sternberg Astronomical Institute, Moscow, Russia; University of Padova, Italy Mikhail E. Prokhorov; mike@sai.msu.ru Sternberg Astronomical Institute, Moscow, Russia Here we review present state of theoretical and observational exploration of isolated neutron stars. ... Gvaramadze, V.V.) 2002, «Neutron stars in supernova remnants and beyond», astro-ph/0212541...

... Average effective wavelengths and band widths for various sp ectra Lyrae spectrum f flat k е 1014 Hz 5386 ± 18 4.66 ± 0.04 5714 ± 12 4.1 6234.5 ± 0.5 1.03 5372 ± 18 4.69 ± 0.04 eff 2 Optical Filter ID 1 2 3 4 a Fo c -6 10 erg/cm2 s 12.55 ± 0.10 11.04 ± 0.01 2.77 ± 0.004 12.63 ± 0.10 fo d 6 10 photons/cm2 s 3.40 ± 0.02 3.18 ± 0.004 0.87 ± 0.002 3.42 ± 0.02 Power-law eff f 2 е 5746 ± 317 6197 ± 253 6305 ± 31 5736 ± 316 spectra pl k 1014 Hz 3.70 ± 0.26 3.14 ± 0.16 0.88 ± 0.01 3.70 ± 0.27 Table 1. ...

Венера - утренняя и вечерняя звезда . ... Исследование Солнечной Системы - Венера . ... Венера . ... Venus Express" . Страница: КА "Venus Express" ( Part #1 , Part #2 ), Выход на орбиту , 2 года у Венеры , Гидроксил на Венере , Действующие вулканы? ... 29 января 2013 стали известны результаты уникальных наблюдений ионосферы планеты в период пониженного давления солнечного ветра. ... У Венеры Venus Express зафиксировал концентрацию 0.2 см 3 , а динамическое давление снизилось до 0.1 нПа. ...

Вы находитесь здесь: Статьи А.А. Волчков. Вывод положений и собственных движений звезд программы Карта Неба . ... Выложена полная версия каталога 2MASS в формате SIMFOV и версия программы, поддерживающая этот каталог. ... С целью устранения этого было решено определять ошибки телескопов совместно с выводом собственных движений, используя в качестве второй эпохи более поздние, чем АК, наблюдения. ... При выводе координат и собственных движений звезд АК использовалось разбиение неба на участки 2*2њ. ...

Главная > Все корабли > Буран > Библиография . ... К 23-летию полета "Бурана" . ... Разговор в ЦПКиО им. М.Горького, сентябрь 2011 г. Программа создания многоразовой космической системы (МКС) 11Ф36 "Буран" была самой масштабной в истории отечественной космонавтики. ... В середине 1970-х годов, на заре программы "Буран", предполагалось, что летать наши многоразовые корабли будут много и часто. ... После принятия этого решения программа полетов "Бурана" переходила к кораблю 2.01. ...

... Meade Instruments Corporation . ... Microscope Instruction Manual . Meade Model 9400 . Meade Model 9400 Microscope Introduction. The Meade Model 9400 Microscope is a precision instrument enabling startling views of the microcosmic world with its all-metal construction, fine glass optical elements, and precision adjustments. ... Your Meade Model 9400 Microscope requires some minor assembly of the Eyepiece, Objective Lenses, and Illuminating Mirror. ... Index of Instruction Manuals . ...

... POLAM-L . ... ABOUT LOMO . ... MICROSCOPES . ... OEM OPTICAL COMPONENTS . ... Home Products Microscopes POLAM-L POLAM-L™ 213-BE . ... Fine / Coarse . ... Stage . ... LOMO America, Inc. will repair or replace the defective microscope covered by this warranty free of charge if it is returned, postage prepaid, to LOMO America's Service Center in Prospect Heights, Illinois in its original package. A Return Authorization Number (RAN) has to be obtained from LOMO America, Inc. prior to shipping. ...