... Behemoth black hole found in an unlikely place . ... galaxies . ... black holes . ... No direct link between black holes and dark matter . ... Massive black holes have been found at the centers of almost all galaxies, where the largest galaxies т??the ones also embedded in the largest halos of dark matter т?? harbor the most massive black holes. This led to the speculation that there is a direct link between dark matter and black holes т?? that exotic physics controls the growth of a black hole. ...

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• Magnetic fields, subatomic particles, etc., traveling in different directions
• Reproducing the large-scale universe | Astronomy.com
• Space weather center to add world's first "ensemble forecasting" capability |

Peremennye Zvezdy ( Variable Stars ) 33 , No. ... We present our discovery a new variable star USNO-A2.0 1350-17086180 from observations at the Astrotel-Caucasus Observatory. ... The numbers of observations on each of the observing nights are presented in Table 1; the observations are attached to the html version of this paper. ... Numbers of observations . ... No. observations . ... 0.001 . ... 0.000 . ... 0.003 . ... 0.004 . ... 0.002 . ... 0.005 . ...

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Preliminary results of astroclimate parameters measurements at the Sternberg 2.5m telescope installation site V.Kornilov, N.Shatsky, S.Potanin, O.Voziakova, B.Safonov Moscow, 2008 Acknowledgements A.Belinskiy M.Kornilov A.Tokovinin M.Kuznetsov P.Kortunov E.Gorbovskoy SAI administration some SAI students Pulkovo solar station (KHSS) staff RFBR support MAVEG Gmbh Why to study optical turbulence and some other relevant ... Mean seeing by DIMM data for this night is 1''5. ...

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• http://curl.sai.msu.ru/mass/download/doc/pmt_param_eng.pdf
• http://curl.sai.msu.ru/mass/download/doc/infrasoft_eng.pdf
• . The . MASS . Group .

... OEM COMPONENTS . ... OEM OPTICAL COMPONENTS . ... Objective, Plan Achromatic, 4 X 0.12, BF . ... Objective, Flatfield Achromatic, 20 X 0.40, BF . ... Objective, Flatfield Achromatic, 60 X 1.00-0.70, Oil, Iris, BF . ... Objective, Flatfield Achromatic, 100 X 1.25, Oil, BF . ... Q-Plan? Achromat Objective, 2.5 X 0.08, BF . ... Q-Plan? Achromat Objective, 50 X 1.0-0.70, oil, iris, BF/DF . ... Q-Plan? Achromat Objective, 100 X 1.25, oil, BF . ... Q-Plan? Achromat Objective, 100 X 1.30, oil, iris, BF/DF ...

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• OEM Optical Components
• Kentaur
• Professional Telescopes

... The described algorithm is suitable for measurements of complex images of stars. ... a) the zero-based number of stars in the complex (multicentric) image, . b) set of preliminary coordinates - x i , y i , for all stars, index i is number of a star, . ... i - index of a star in the complex image; . ... These parameters are calculated by a nonlinear method of a least squares.The main output parameters of this algorithm are x i , y i ; where the index i is number of a star in the multicentric image. ...

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The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . ... Listed Since October 22, 1998 . ... 203) 484-7705 . ... 203) 484-9016 . Web Site . ... Web . www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• S.T.A.N.O. Components Inc., AstroGuide Listing
• The Destropic Principle - an Astronomy Net God Science Forum Message
• Observational Stellar Astronomy - an Astronomy Net Article

Solar Phys (2012) 276:97ґ112 DOI 10.1007/s11207-011-9883-6 Investigation of Hot X-Ray Points ( HXPs ) Using Spectroheliograph Mg XII Experiment Data from CORONAS-F/SPIRIT A. Reva Ї S. Shestov Ї S. Bogachev Ї S. Kuzin Received: 10 May 2011 / Accepted: 18 October 2011 / Published online: 24 November 2011 ? Springer Science+Business Media B.V. 2011 Abstract Observations in the Mg XII 8.42 е line onboard the CORONAS-F satellite have revealed compact high ... Figure 7 Intensity variation of HXPs. ...

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• Publications
• Publications - 2006

The low aspect ratio, or spherical tokamak Globus-M [1] has recently been built in a support of international spherical tokamak plasma investigation program. ... The survey to determine the work scope in diagnostic design for Globus-M is given in the paper. ... The next one is an advanced diagnostic set intended to supply the data on basic plasma parameters: electron temperature and density profiles, ion temperature, plasma composition, radiation profile, Zeffective. ... Magnetic Diagnostics. ...

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Общая Астрономическая Конференция > Практика > Астрономический наблюдательно-информационный портал > Хвостатые гостьи (все о кометах) . C/2011 J2-B (LINEAR) _ CK11J02b, ранее B component - отделившаяся часть ядра кометы C/2011 J2 (LINEAR) .. ... C/2011 J2-B (LINEAR) _ CK11J02b, ранее B component - отделившаяся часть ядра кометы C/2011 J2 (LINEAR), К -1, M -1, M -2, # 220 , # 3 , # 1 , # 6 , CBET 3979 , CBET 3986 . ... Элементы орбиты C/2011 J2-B (LINEAR) _ CK11J02b (ранее B component): . ...

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• Общая Астрономическая Конференция - Показать сообщение отдельно - Хвостатые
• P/2010 V1-F (Ikeya-Murakami) _ PK10V01f - фрагмент Ф (component F)
• P/2010 V1-D (Ikeya-Murakami) _ PK10V01d - фрагмент Д (component D)

... According to the estimations of the RSC Energia it will take at least 10 years and 500-600 million $ (cost of adjustment, preparation, equipment's launching and accompaniment of carrying out of the experiments is included) to build up a similar experimental complex. ... It was carried out successfully. ... Radiation researches on the station Mir, carrying out by Moscow State University, gave rise to the construction of the dynamic picture of radiation zones' changes during the sun activity cycle. ...

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... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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• VISTA - Visible and Infrared Survey Telescope for Astronomy

... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...

73. http://vast.sai.msu.ru/lk/