. This is a new popup window - close it when you are done . Submitted by Mario Motta M.D. on 04/04/2015 17:42:43 . IC 4050 . the inner part of the "flame nebula" . Logon to post a follow-up comment or review comments from others . Copyright (c) Amateur Telescope Makers of Boston, Inc. About Us Contact Us

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... The TESIS is a set of solar imaging instruments developed by the Lebedev Physical Institute of the Russian Academy of Science, and launched aboard the Russian spacecraft CORONAS-PHOTON on January 30, 2009. The main goal of the TESIS is to provide complex observations of solar active phenomena from the transition region to the inner and outer solar corona with high spatial, spectral and temporal resolution in the EUV and Soft X-ray spectral bands. ... Solar activity hits a new low . ...

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• Double Engine Fuels Star's Remarkable Nebula - Astronomy news

. XMM-Newton Science Analysis System . omsource (omsource-1.15.5) [xmmsas_20070708_1801-7.1.0] . Meta Index / Home Page / Imaging Mode Photometry Window / Annuli controls This spin-box determines the semi-major axis of the inner background annulus. XMM-Newton SOC/SSC -- 2007-07-09

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... STScI-PRC95-45a CRUCIBLE OF CREATION: PANORAMIC HUBBLE MOSAIC ZOOMS IN ON MAELSTROM OF STAR BIRTH This spectacular color panorama of the center the Orion nebula is one of the largest pictures ever assembled from individual images taken with NASA's Hubble Space Telescope. ... Though this 2.5 light-years wide view is still a small portion of the entire nebula, it includes almost all of the light from the bright glowing clouds of gas and a star cluster associated with the nebula. ...

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• WISP Observations of the Pleiades in the Ultraviolet
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... Several attempts to discover the FICN signal in VLBI nutation series made during last years failed. ... We investigated several VLBI CPO series by means of spectral and wavelet analysis. It has been shown that there are several periodic signals with close amplitude around the expected FICN period without any prevailing one that can be reliably associated with the FICN. ... DATA ANALYSIS We analyzed several CPO series obtained in IVS analysis centers by means of spectral and wavelet analysis. ...

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• Formation of the Solar System
• How a Nuclear Reactor Works
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... On February 9, 1986, the most famous comet of all time will make the closest approach to the Sun in its current 76-year trip around our star. ... Why is the comet named Halley ? Is Comet Halley on target for its rendezvous with the inner solar system? ... These comets then move around the solar system in huge elongated orbits, which means they spend most of their time far away from the Sun. ... The coma and tail of a comet, indicated on a photograph of Halley's Comet taken on May 8, 1910. ...

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• ASP: Lord of the Rings
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... 8, ``Celestial Mechanics'', 2002 Investigation of stability of NEAs orbital resonance motions by numerical methods L. E. Bykova Tomsk State University, Tomsk, Russia The problem of orbital stability of resonance Near­Earth asteroids (NEAs) is considered. Most of NEAs have multiple close approaches to the inner ma­ jor planets. ... The technique of the investigation of NEAs orbital stability has been devel­ oped by author on the basis of the construction of possible motion domains (R) of asteroids. ...

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• http://www.ipa.nw.ru/conference/2002/sovet/PS/GALUSH.PS
• Keywords_52

... autoOutline (int startX, int startY) . ... 0 and the boundary points can be accessed in the public xpoints and ypoints fields. public void autoOutline (int startX, int startY, double lower, double upper) . 0 and the boundary points can be accessed in the public xpoints and ypoints fields. public void autoOutline (int startX, int startY, int lower, int upper) . This is a variation of legacy autoOutline that uses int threshold arguments. public void autoOutline (int startX, int startY) . ...

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... Главная страница / Кометы и астероиды / "Нас не догонишь". Комета 217P/LINEAR, M42, M43, Бегущий Человек и пролетающие спутники. ... M42 , M43 , БегущийЧеловек , 217P/LINEAR . ... Комета C/2009 R1 (McNaught) . ... Все права на размещенные в галерее фотографии принадлежат их авторам. ... Киевский клуб любителей астрономии "Астрополис" . Движок галереи: 4images 1.7 ...

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Планета Земля и Луна . ... Космическая защита . Луна . Фотографии . ... Строение Луны . ... Страница: Начало одиссеи , Экспедиции , Море Кризисов , "Аполлон-8" , "Аполлон-9" , "Аполлон-10" , "Аполлон - 11" , E-8 "Луноход" , Испытания Л-1 , Луноход - 1,2 , КА "Луна 1-24" , КА "Луна-9" , Луна от КА СССР ; . Луна - наш космический спутник . ... Снимки Луны от аппаратов серии Луна и Зонд (СССР) . Фотографии космических аппаратов серии "Луна" (также Луноходы) и "Зонд" - СССР . ... Зонд 3 . ...

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God Science Forum Message . Forums: . ... God and Science ћ SETI ћ Software ћ UFO ћ XEphem . ... Discussion Forums | God and Science | ... Right Next To You.. Pay Atention!! Forum List | ... Post Message | ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Harvest Moon - an Astronomy Net Article
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... 145Kollgaard+ A 29.3 deg^2 region surrounding the north ecliptic pole (NEP; RA=18h00m, dec = 66^o30') was mapped with VLA at 1.5 GHz to support the deepest portion of the ROSAT all-sky soft X-ray survey. The resulting VLA-NEP survey catalog contains 2435 radio sources with flux densities in the range of 0.3-1000 mJy, including over 200 fainter than 1 mJy. ... Between 1 and 150 mJy the slope of the logN - logS relation is 0.68+-0.03. ... Table 2 gives the resulting VLA-NEP source catalog. ! ...

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... Eclipses in the double--binary pulsar PSR J0737-3039 A/B . In the binary radio pulsar system J0737-3039 the faster pulsar A is eclipsed once per orbit while the slower pulsar B shows orbital-dependent variations of intensity. ... We construct a model of eclipses which reproduces the observed light curve up to intricate details and proves the long standing assumption of dipolar magnetic fields of neutron stars. ...

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The sky window shows the position of the telescope and the user's catalog objects on the sky (the inner az/alt polar grid) and also the position of the azimuth axis along its wrap (the outer spiral). ... The target position of the telescope (where it will end up after the slew) is shown as a plus. ... The potential position of the telescope (the position in the Slew window ) is shown as an X. Objects in the users's catalog (those with alt>0) are shown as dots. ...

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• Preparations for science:
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• emerg_close

Laboratory of Stellar Physics . ... A study of close binaries with black holes, neutron stars and white dwarfs. ... A study of SS433 - the massive close binary with a black hole in the regime of supercritical accretion . ... A search for intermediate-mass black holes (IMBH). The black holes which are not supermassive black holes observed in quasars, and which were formed not in massive stars. ... A search for new magnetic stars, new CP stars, measurements of magnetic fields in stars . ...

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... The analysis shows, that asteroid ­ rubble pile loses its fast fragments in no time but the retaining fragments forms a compact structure immersed in dust ­ gas atmosphere, created by interaction of interplanetary medium with dispersed product of collisional evolution of asteroid. By interaction of an asteroid ­ rubble pile with interplanetary medium structures asteroid can increase its brightness on account of blowed up dust simulating phenomenon of distant comet's brightening. ...

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• http://selena.sai.msu.ru/Shev/Publications/m44_75_shevchenko_etal.pdf

... Fix $s$ with $Re (s)=\sigma$, and let $\chi$ run over all Dirichlet characters with (say) prime conductors. Then (generally conjecturally), $M_{\sigma}(z)$ (resp. $\tilde{M}_{\sigma}(z)$) coincides with the limit-average over $\chi$ of $\delta_z(L'(\chi,s)/L(\chi,s))$ (resp. $\psi_z(L'(\chi,s)/L(\chi,s))$). Here $\delta_z(w)$ is the Dirac measure concentrated at $z$ and $\psi_z(w)=\exp(i Re(\bar{z}w))$ is the additive character on the field of complex numbers parametrized by $z$. ...

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• Conference "Zeta Functions"
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... 2000: . The images and maps of polarization for a massive protostar S140 IRS1, immersed in a dark molecular cloud were obtained at the 6-m telescope using speckle interferometry in the infrared 2.2 micron band. According to the structure of the flocky envelope around the nascent star it was found that the bright emission was caused by the reflection of radiation from the inner walls of the cavity formed by a powerful molecular outflow from the protostar. ... Archive . ...

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• Galaxy sector, archive 2004
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• Galaxy sector, archive 2002

Journal of the Amateur Astronomers Association of New York October 2008 Volume 56 Number 10, ISSN 0146-7662 EYEPIECE ysis of Cassini pictures. ... Saturn's 60 moons are divided into inner and outer groups. ... There are a diverse group of worlds such as Tethys, Dione, Rhea and Mimas, the latter known as the Death Star moon for its uncanny resemblance to the Star Wars movie's battle station. ... The strange planet so far from its parent star is unexpected based on theories of star and planet formation. ...

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• http://www.aaa.org/EyepieceFiles/aaa/2009_09_September_Eyepiece.pdf
• http://www.aaa.org/EyepieceFiles/aaa/2015_03_March_Eyepiece.pdf
• http://www.aaa.org/EyepieceFiles/aaa/2010_02_February_Eyepiece.pdf