... Membership . ... The name of this organization shall be Amateur Astronomers Association of Princeton, Incorporated (hereinafter abbreviated as AAAP). ... General membership shall be open to any person paying dues with the proviso that any member under the age of 18 must be accompanied by a responsible adult while at any AAAP meeting, other function, or observatory. ... A. Director The Director shall preside at all meetings of the Board of Trustees and at all general membership meetings. ...

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... 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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• Second Spectrum-RG/eROSITA Conference

Properties of the Solar Eruptive Event of 19 October 2001, 09:40 UT . ... 1) IZMIRAN, Troitsk, Moscow Region, 142190 . ... Basing on IZMIRAN and NIRFI radio observations, we analyze an event which is characterized by sufficiently intense emission in the cm- and dm-ranges under almost total lack of metric bursts. This peculiarity appears to be caused by very slow speed (V~240 km/s) of a coronal mass ejection (CME) recorded in this event with SOHO/LASCO. ... Coronal Mass Ejections . ...

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• Heliophysical Laboratory of IZMIRAN (Solar-Terrestrial Physics Division)

... New technique measures mass of exoplanets . ... Now, scientists at the Massachusetts Institute of Technology (MIT) have developed a new technique for determining the mass of exoplanets using only their transmission spectra dips in light as a planet passes in front of its star. ... To determine the mass of an exoplanet using transmission spectroscopy, de Wit relied on the effect that a planet s mass has on its atmosphere, as transmission spectra give information on a planet s atmospheric properties. ...

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... I. Mean Surface Brightnesses and Integral Color Indices for Bars Gusev A.S. ================================================================================ Abstract: UBVRIJHK surface brightnesses and color indices of bars of galaxies are determined using surface photometry data for 100 barred galaxies (table1.dat). ... J0 Mean surface J0 brightness 46 A1 --- CI- CI sign 47 -50 F1.2 magn/sq.arcsec. U-B)0 (U-B)0 color index 52 -55 F1.2 magn/sq.arcsec. ...

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• Division of the Galaxy and Variable Stars
• V.Surdin's List of Scientific Publications
• Data bases of Natural Satellites. Documentation. Structure

Prague, August 16, 2006 . Our trial revision of the GCVS data for several southern constellations show that type changes are not needed for most stars. ... We suggest to add one more symbol combining types, in the cases when two or more classification options remain for the same star, for example, EC|Ell, EC|RR (here EC means a contact eclipsing binary, this is one of our suggestions from next slides). ... Moreover, it will simplify moving stars from the suspected-variable catalogue to the GCVS. ...

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Общая Астрономическая Конференция > Товары для астрономов > Полезное для астрономии . Проблемма с EQMOD . ... Поиск . Сообщения за день . ... V_Udo . ... Найти еще сообщения от V_Udo . ... Созвездия (поиск и описание) .. Созвездия южного неба (поиск и описание) .. Осенние созвездия (поиск и описание) .. Летние созвездия (поиск и описание) .. Околополюсные созвездия (поиск и описание) .. Весенние созвездия (поиск и описание).. Зимние созвездия (поиск и описание) .. ...

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• Проблемма с EQMOD [Архив] - Общая Астрономическая Конференция

. Distance Conversion Calculator . by Matt Oltersdorf 2000 04 02 2225 UTC . Type the known value into the appropriate units field, click the . calculate button and the program will show all values for . related unit properties. Kilometers . Meters . mm . Inches . Feet . Yards . Miles . Astronomical Units (A.U.) . Light Year (LY) . Parsec (pc) . Kilometers . Miles .

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... Bad Astronomy . ... Bitesize Astronomy . ... Keep Bad Astronomy close to your heart, and help make me filthy rich. ... Right now as I write this, the planet Venus shines brightly in the evening sky, getting higher with each passing day. ... Actually, when astronomers were first able to start measuring properties of Venus, it did look very much like a twin of Earth. ... 2008 Phil Plait. ... Subscribe to the Bad Astronomy Newsletter! Talk about Bad Astronomy on the BA Bulletin Board! ...

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• Phil Plait's Bad Astronomy: Bitesize Astronomy
• Phil Plait's Bad Astronomy: Bad TV

... Planets . ... Exoplanets . ... After the discovery of powerful telescopes we were able to see further into our Solar System and discover many distant objects and dwarf planets.€а However within the last 16 years astronomers have started to dedicate much more time to the search of other worlds in orbit around other stars beyond the realm of our Solar System. ... However the closest star with a known exoplanet is the star Epsilon Eridani which is a mere 10.4 light years away from planet Earth. ...

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• Star Older Than the Universe | Astronotes

... Pulsars offer a variety of observables for study of interstellar scattering. Observations of scattering of nearby pulsars and intra-day variable quasars point to the existence of a component of the interstellar medium (ISM) which has properties quite different from the more distant, diffuse ISM. ... The time series of electric field emitted by the pulsar is convolved with an impulse-response function due to scattering, when sampled at the observer plane [1]. ... Nearby interstellar scattering. ...

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• http://www.asc.rssi.ru/RadioAstron/meetings/RUni_Oct2008/abstracts.pdf
• http://www.asc.rssi.ru/RadioAstron/meetings/RUni_Oct2008/agenda.pdf
• http://www.asc.rssi.ru/RadioAstron/publications/articles/tmp/evn%202014_065.pdf

. This Directory contains Model of distribution of density, temperature and effective collision freguency of electrons. Yu.K.Chasovitin. 1998. This Directory contains The program RIM98 for calculating the parameters of the ionosphere to use the "Reference Ionospheric Model-98" (RIM-98).Yu.K.Chasovitin. 1998.

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• "STP Data" STP Data
• Catalogue 5 of WDC-B

... Moon Phase below . ... ARTICLE: Why the moon always shows us the same face . ... Before you continue reading, you should know that this was not always the case, i.e. the Moon once was rotating with respect to the Earth, so that on every night a terrestrial observer (if there was one, because this was long, long before mankind appeared on our planet, and even before any major animals had appeared) saw another face of the Moon. ... Figure 1 (not to scale) shows how we can imagine the system Earth-Moon...

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... Schools . School of Biology . ... Dean?s Office . Departments . ... University History Museum . ... School of Physics . ... Crystal Physics Department . ... It was opened at the department for practical training improvement of students and for further research development in Physics of functional materials (University order ? ... Study groups from Germany (University of Duisburg-Essen) and our department that since 2000 work closely in Physics and Chemistry of biomaterials, on Symposium, 2010. ...

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... Ниже приводится код данного класса: DBClass.cls Option Explicit Private WithEvents ConRs As ADODB.Recordset Private dbConn As ADODB.Connection Private mvarConStr As String Private mvarSQLStr As String Private Sub Class_Initialize() Set dbConn = New ADODB.Connection End Sub Private Sub Class_GetDataMember(DataMember _ As String, Data As Object) Set Data = ConRs End Sub Public ... Создадим на форме один текстовый блок Text1 и присвоим его свойству Index значение 0. ...

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ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: RECENT PROGRESS AND NEW HORIZONS 4-th GAMOW INTERNATIONAL CONFERENCE IN ODESSA and 9-th GAMOW SUMMER SCHOOL Astronomy and beyond: Astrophysics, Cosmology, Radioastronomy, High Energy Physics and Astrobiology 17-23 August , 2009, Odessa, Ukraine EVENTS: Monday, 17.08.2009 Arrival 09.00 ­ 22.00 Registration of participants Tuesday, 18.08.2009 05.59 09.00 10.00 11.00 13.00 13.15 14.30 16.00 ...

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• http://www.astro-soc.odessa.ua/Program-2006.pdf
• http://www.astro-soc.odessa.ua/Public-2011.pdf
• http://www.astro-soc.odessa.ua/Public-2010.pdf

... ORAL SESSION . ... Registration /Coffee . ... Sergey Bogachev : Space solar investigations in the Lebedev Institute: from Sputnik-2 to future missions . ... Splinter session. S1 : SOLARIS mission proposal (chair - S.Kuzin) . ... Morning Coffee . ... The Sun from radio to gamma rays: new results from space and ground-based observatories (part 1) . ... Szymon Gburek : SphinX and XRT observations of active regions . ... Artem Ulyanov : Nanoflares in the quiet solar corona: a view from SDO/AIA . ...

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... For the past years I have been working on the problem of synthesis of light curves of close binary systems, consisting of a normal star and a compact object (point object with fixed X-ray luminosity). ... Possible existence of a bright spot on the disk's lateral surface is taken into account. ... The last of then will be published in Gordon and Breach Publishers ( Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ... Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ...

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• Irina Glushneva

... Горизонты науки о Вселенной (Модераторы: Дмитрий Вибе , AlAn ) ? что есть поле и что есть время? . ... Ответ #60 : 20.01.2003 [18:31:18] ? ... Записан . ... Рейтинг: +26/-12 . ... Вы правы ответ уж больно очевиден. ... Ответ #66 : 07.06.2006 [08:16:54] ? ... В голове не укладывается, вы уж извините: Не говорит ли такая бесструктурность поля о какой-то единой связи всей материи во Вселенной? ... Это из моей статьи "The Mathematical Justification of a Possible Wave Nature of the Time . ...

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• arxiv:0704.0889 Библиометрические статистические свойства 100 крупнейших европе
• arxiv:0903.2260 Физические параметры красного сверхгиганта WOH G64: самая
• arxiv:1504.02165 Определение источников перитонов на телескопе Паркс - Научная

... 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. ...

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• http://master.sai.msu.ru/media/presentations/2014/20140208_Shibata.pdf
• http://master.sai.msu.ru/static/YaB_100/20/Khlopov.pdf