Вы находитесь здесь: Каталоги Подключение каталогов к SIMFOV . ... Каталоги для программ-планетариев . ... Для подключения нового каталога, прежде всего, необходимо создать текстовый файл , содержащий по одной строке, на объект, оканчивающейся двухбайтовым символом Enter (если только таковой файл отсутствует). ... В настоящий момент звездная величина в каталогах типа OTHERS программой SIMFOV не используется, но выдавать ее можно из файла *.Dat , включив звездную величину в формат выходной информации. ...

Композиты и наноструктуры COMPOSITES and NANOSTRUCTURES ?3 2009 СОДЕРЖАНИЕ А.Р. Банселл, А. Тионнэ, С. Камара, Д.Х. Аллен Накопление повреждений и оценка долговечности углепластиковых сосудов высокого давления .. ... 2009 3 ?3 2009 Композиты и наноструктуры COMPOSITES and NANOSTRUCTURES CONTENS A.R. Bunsell, A. Thionnet, S. Camara and D.H. Allen Damage accumulation and life prediction in carbon fibre composite pressure vessels .. ... International Conference on Composite Materials ICCM-17. ... 2009 4 ...

... SMIS ] . Composite Image of Cloudiness over Russia . Satellite passes used for composition: . NOAA 18 -- 09.04.2016, 06:56 GMT . ... NOAA satellite data used for image composites, have been received and processed by satellite receiving center at Institute of Solar-Terrestrial Physics (Russian Acad.Sci., Siberian Branch, Irkutsk ) and Space Monitoring Information Support Laboratory (SMIS IKI RAN, Russian Acad.Sci., ... Back to SMIS Home Page . ...

... Информация Объявления В Москве пройдет финал I Открытого чемпионата России по композитам Composite Battle-2015 . ... 28-29 октября в Москве на форуме Открытые инновации пройдет финал I Открытого чемпионата России по композитам среди молодых специалистов предприятий и студентов вузов Composite Battle-2015. ... Финал I Открытого чемпионата России по композитам пройдет в формате workshop, что даст участникам возможность продемонстрировать свое практическое умение работать с композиционными материалами....

... Keck spectropolarimetry, giving spectral coverage from Ly- to beyond CIII], and HST imaging of a sample of powerful radio galaxies with has been obtained. ... This is a short progress report on a rather extensive programme we are carrying out to study the structure and composition of high redshift radio galaxies (HzRG) -- and, by implication, the host galaxies of radio quasars -- using observations in the optical, IR and mm bands. ... An example of the NICMOS and WFPC 2 imaging is shown in Figure 2 ...

... More than 300 surface reconstructions are already known for pure Si surface and Si surface with adsorbate. Study of their properties by the methods of surface physics reveal numerous interesting phenomena including various phase transitions accompanied by changes of Fermi-surface topology, development of the charge-density wave, etc . ... The charge-density wave (CDW) develops in materials with a chain-like crystal structure at temperatures below the Peierls transition temperature. ...

. Cosmology . Very Early Universe . Cosmic Microwave Background Anisotropy . Dark Matter Models . Large Scale Structure . High Energy Astrophysics . Active Galactic Nuclei . Astrophysics of Compact Objects . Accretion Disks . Scientific Staff:

... 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. ...

Download Izmccd (~2.7 MB). Solution of problems at identification of star field. ... 2) Scale is not correct. ... In this case algorithm of identification will revise all values of scale from twice smaller up to twice greater. ... There should be more than value of the field "Number of stars in frame". ... The star field is considered identified if number of the identified stars more or equally to this value. It is necessary to set value from 4 up to value of field "Number of stars in frame". ...

Альтернативный форум . Scientific.ru Все форумы . ... Time (@) - 13.04.2007 09:15 . Re: Anisotropy in the Hubble constant as observed in the HST Extragalactic Distance Scale Key Project results . x203a; x203a; x203a; в ответ на: Anisotropy in the Hubble constant as observed in the HST Extragalactic Distance Scale Key Project results Котофеич . ... Re: Anisotropy in the Hubble constant as observed in the HST Extragalactic Distance Scale Key Project results Котофеич, 13.04.2007 13:37 . ...

... Произведение двух точных квадратов является точным квадратом. Если два целых числа представимы в виде суммы двух квадратов, то их произведение тоже представимо в виде суммы двух квадратов. ... Дальше стоит немного уточнить задачу: дело в том, что по теореме Лагранжа любое натуральное число представимо в виде суммы четырех (а значит, и большего числа ? ... Соответствующие алгебры суть вещественные числа R , комплексные числа C , кватернионы (числа Гамильтона) H и октавы (числа Кэли) O .) ...

... Uniformity of size and appearance of all the illustrations of the same type should be strictly observed. ... The numbers of curves, straight lines, etc., should be written in italics without any brackets both at an illustration and in text. ... In inscriptions, when the parameters of a curve are listed, the numbers of curves and notations of the parts of an illustration (a, b, etc.) should be placed in brackets prior to the corresponding parameters (a dash is not used). ...

The LCDM paradigm: successes and challenges on scales of galaxies Anatoly Klypin (NMSU) LCDM · · · · DM profiles, concentrations, .. Clustering of galaxies: P(k) and correlation functions Satellites: abundance, number-density profiles Galaxies and Dark Matter: abundances Dwarfs. ... Springel et al 2008. ... Klypin et al 2010. ... Observations - LCDM: just enough Magellanic Clouds Observations LCDM Vmax > 50 km/s Busha et al 2010 Dark matter profiles: standard LCDM Aquarius simulation. ...

... Seminar archive . ... Seminar archive 2011 3 June . ... Tristram K. D. A torus of molecular gas and dust is one of the key components of unified schemes of active galactic nuclei (AGN): it provides the material for accretion onto the supermassive black hole and is held responsible for the orientation-dependent obscuration of the central engine. I will present the results and current status of infrared interferometry of these dust distributions in AGN in the infrared. ... All seminars: . ...

... How to Find Us . ... Take a stroll around the beautiful grounds of the Armagh Observatory Astropark. Armagh Observatory's Astropark is a scale model of the Universe where visitors can walk through the Solar System and into the Milky Way and beyond. The landscaped grounds are dotted with stainless steel scale models of the planets demonstrating how small our planet Earth is compared with some of its neighbouring worlds. ... Find out more about the Armagh Observatory Astropark. CONTACT US . ...

Lvov 2001 . Musical Kp diagram 2001 (*.pdf) . ... Horizontal intensity - H. Vertcal intensity - Z. from 0h. 00m. 1.01.2001 to 24h. 00m. 31.12.2001 . ... from 0h. 00m. 1.01.2001 to 24h. 00m. 31.08.2001 . ... from 0h. 00m. 1.01.2001 to 8h. 00m. 12.04.2001 . ... from 8h. 00m. 12.04.2001 to 8h. 45m. 25.05.2001 . ... from 8h. 45m. 25.05.2001 to 24h. 00m. 31.12.2001 . ... from 0h.00m.1.01.2001 to 24h.00Л.31.12.2001 . 0.50 min/mm . ...

Rastorguev А.S. "Astronomical Distances" (Lecture course for postgraduates, 2009-2016) . Part 1. ... Trigonometric parallaxes of stars. Moving clusters distances. ... Photometric distances: general approach. Normal stars as "standard candles". ... Main Sequence fitting or distance scale of star clusters. ... Moving photospheres technique. Cepheid distance scale and P-L relations. RR Lyrae distance scale. ... Globular clusters luminosity function. ...

MSU-E data examples. ... MSU-E . ... 16/03/1995 10:40 Msk . Pseudo-colour image. Red - channel 3, Green - channel 2, Blue -channel 1 . scale of projection 40 m/pixel . ... True-color image (786486K) . ... Channel 4 . ...

... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...

... I am involved in Project Astro, a program to bring astronomers into public schools to assist with teaching students about science and astronomy. ... While there are all sorts of scale model of the Solar System type exercises ( Mitchell Charity's page has a good listing of what's available), none were really tailored towards discovering the spatial relationships of the planets, and in a way that could be done at night as part of a Star Party. ...