ПУБЛИКАЦИИ - 2010 год . ... Зависимость величины Форбуш-понижений от параметров солнечных эрупций. 31-я Всероссийская конференция по космическим лучам, МГУ, Москва, 5-9 июля 2010 г. Доклад опубликован в электронном виде на флэш-диске 'Материалы 31-ой Всероссийской конференции по космическим лучам, МГУ, Москва, 5-9 июля 2010 г.', файл MOD_07.pdf и доступен по адресу: http://cr2010.sinp.msu.ru/cr2010/mod/mod_07.pdf Презентация доклада доступна по адресу: http://cr2010.sinp.msu.ru/presentations . ...
ЗАО "Звездный Альманах" представляет! Уникальная услуга - купить звезду в подарок! ... Звезда Дня рождения . ... Звезда Любви . ... Купить звезду в подарок на день рождения, на первый взгляд, весьма необычное желание, однако с компанией Звездный Альманах оно вполне осуществимо. ... Особенности Звезды ?Дня рождения? (подарок на торжество) заключаются в том, что координаты звезды наиболее точно соответствуют ее местоположению в зодиакальном созвездии на число и месяц рождения человека ? ...
... Метеориты . ... Астрономия . Всемирный календарь . ... Метеоритика и астрономия". В предлагаемом сайте собраны материалы о метеоритах, полученные в экспедициях Красноярского отделения Российского Астрономо - Геодезического Общества (РАГО) и астрономического кружка станции юных техников города Железногорска Красноярского края, а также различные публикации на эту тему. Автор сайта: Леонид Асочаков. ... Чтобы познакомиться с темой нажмите на кнопку с ее названием и далее на название статьи. ...
The table below (see ASCII version ) lists all known pulsars in globular clusters with the original references whenever available. ... Total number of pulsars: 146, in 28 globular clusters . ... EPN pulsar database . ... Cluster/Pulsar . ... 47 Tuc (NGC 104) . ... mildly eccentric . ... low-mass . ... 0.0 . ... The maximum pulsar mass is 2.52 M ? ... Only one Galactic MSP has an eccentric orbit (PSR J1903+0327), all other eccentric binary pulsars with spin periods below 20 ms are in globular clusters. ...
... Проф. А.Д.Чернин (ГАИШ, МГУ, Москва): ЭНЕРГЕТИЧЕСКИЙ СОСТАВ ВСЕЛЕННОЙ: НОВАЯ СИММЕТРИЯ 13.00-15.00. ... Проф. Л.И.Мирошниченко (ИЗМИРАН, Троицк, Россия): СОЛНЕЧНОЗЕМНЫЕ СВЯЗИ В 23-ЕМ ЦИКЛЕ СОЛНЕЧНОЙ АКТИВНОСТИ Лекция 9 10.50-11.30. ... М.И.Рябов, А.Л.Сухарев (Одесская обсерватория Радиоастрономического института НАНУ) : О ПРОЯ ВЛЕНИИ ИЗМЕНЕНИЙ СТРУКТУРЫ ПЕРЕМЕННО СТИ ПОТОКОВ ВНЕГАЛАКТИЧЕСКИХ РАДИОИСТОЧНИКОВ 3С120, OJ287, 3С273, 3С279, 3С454.3 НА РАЗЛИЧНЫХ ФАЗАХ АКТИВНОСТИ 4. ... РИ НАНУ Гравиметр. ...
... We thank the Swift team for their rapid scheduling of this observation. ... 2455705.20851 V 14.15 0.03 2455707.83079 V 14.10 0.03 2455710.84028 V 13.53 0.02 2455713.64631 V 13.66 0.02 2455714.65479 V 14.11 0.03 2455714.71823 V 14.12 0.02 2455714.78596 V 14.20 0.02 2455717.39593 V 14.37 0.03 2455726.62861 V 14.83 0.04 2455727.16343 V 14.57 0.04 2455730.50586 V 14.57 0.03 2455730.57329 V 14.56 0.03 2455730.70360 V 14.66 0.04 2455738.32865 V 14.00 0.02 2455742.86146 V 14.21 ...
lsst.tcc љ 1.2.2-3-g89ecb63 . ... Namespaces . ... NamespaceљList . ... axis . oneSlewIter . ... tcc.axis.oneSlewIter Namespace Reference . ... Compute a slew for all axes, given the starting and target paths. ... slew this axis? A sequence of NAxes bools . ... pathList: a list of NAxes pvtLists, where each pvtList is a list of PVTs describing the motion of that axis; if doAxis[axis] is false then pathList[axis] is an empty list . ... list tcc.axis.oneSlewIter.__all__ = ["oneSlewIter"] . ...
... We present an analysis of an optical blue spectrum of the pulsating helium star V652 Her (=BD+13 3224$) in order to determine its effective temperature, surface gravity and chemical composition. ... The surface composition is characterised by abundances of nH=0.009, He=0.988, nC~0.000040, nN=0.0025 and nO=0.00010 (number fractions). ... If V652 Her was formed by the merger of two white dwarfs, its surface composition demands that they should both be helium white dwarfs. ...
... For reliable estimation of the accuracy of asteroid CCD observations we usually consider from ten or more various NUMBERED MINOR PLANETS (NMPs) observed during several nigths per month (more then 50 positions). ... They can be considered as an indicator of accuracy of the CCD positional observations with given MPC code. ... For any NUMBERED minor planet the (O-C) values must be zero if the errors of observations and the errors of its theory are absent. ...
... Archives . ... You would think that something like ?measurement error? is a well-defined concept, and everyone knows what it means. ... Now?I have more or less a measurement of 1.00+-0.03 Jy for each scan/shot and I?d like to average the values in order to give out a single value for my source. ... So at the end of the run, you have measurements { fi ~ N(1,0.03), i=1..10}, where 0.03 is due to photon noise (i.e., just the statistical error, which I would call the measurement error). ... Chandra Blog...
... 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. ...
... Planets . ... Stars . Exoplanets . ... Most exoplanets so far discovered fall into the category of тАШhot JupitersтАЩ, these are giant planets orbiting very close to their parent star. ... Note that we have discovered so many hot Jupiters because they are the easiest type of planet to find, they are not necessarily particularly common in the galaxy. ... Subsequently several similar hot and€а fuzzy worlds have been discovered the same way, proving this that this planet is not a one-off oddball. ...
Next: Identification and Analysis of Binary Star Systems using Probability Theory . ... We present a computing code for modelling energy flux distributions, photometric indices and spectral line profiles of (non-)radially pulsating Main-Sequence stars. ... In the case of slowly rotating stars one can use the zero-rotation approximation to describe stellar pulsations. Such a model was used already by Cugier, Dziembowski & Pamyatnykh (1994) to study nonadiabatic observables of Cephei stars. ...
... Module pynifs . ... source code . ... Adds a variance array to a pre-existing fitscube instance. source code . ... Returns: data - A fitscube instance identical to the input fitscube, but with the new variance data. source code Function to simultaneously load a variance array and a pixel quality mask into a pre-existing fitscube instance. ... Returns: data - A fitscube instance identical to the initial instance, but with the new variance array and pixel quality mask. source code . ... Returns: Nil. ...
... POLAM-L . ... ABOUT LOMO . ... MICROSCOPES . ... OEM OPTICAL COMPONENTS . ... SURGICAL MICROSCOPES . ... Home Products Microscopes POLAM-L . ... The POLAM?- ... The 360° rotatable head features a built-in iris diaphragm, optical path selector and a vertical photo/video port. ... Microscopes, the stand allows attachment of all the standard and optional modules and components such as stages, condensers, illuminators, intermediate module, and LOMO’s unique, rotatable Monochrometer . ... STAGES . ...
... exoplanets . ... Ground-based detection of super-Earth transit paves way to remote sensing of small exoplanets . ... The transit of exoplanet 55 Cancri e is the shallowest detected from the ground yet, and the success bodes well for characterizing the many small planets that upcoming space missions are expected to discover in the next few years. ... Until now, the transits of only one other super-Earth, GJ 1214b circling a red dwarf, had been observed with ground-based telescopes. ...