... Mass . 17a. Measuring Mass . ... A medium-size (1.25 inch wide) binder clip, as is used in offices to hold papers together--the type made of flat blue steel, with two wire handles. ... The theory predicts that the oscillation period should be proportional to the square root of the oscillating mass, including the mass of the clip. Note that gravity plays no part here: the oscillation period would be the same on the Moon or in zero-g. Denoting square root by SQRT, we have . ...

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• Space Research Institute (IKI) Seminar
• Main results of the experimental and theoretical research completed in 2010
• SKA-3 Results Page

... 8, ``Celestial Mechanics'', 2002 Dynamic evolution of resonance orbits of exoplanets in system 47 Uma B. R. Mushailov, A. A. Kaloshin Sternberg Astronomical Institute, Moscow, Russia The orbits of the major and minor planets of the Solar system indicate that their dynamic evolution is essentially influenced by the effects of orbital reso­ nance interactions. ... One may expect that the orbital resonances can exist not only in the Solar system, but also in other star systems. ...

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• http://www.ipa.nw.ru/conference/2002/sovet/PS/BORDOVIT.PS
• http://www.ipa.nw.ru/conference/2002/sovet/PS/PROKHOR.PS
• http://www.ipa.nw.ru/conference/2002/sovet/abstact/BORDOVIT.TEX.txt

... In Fig. 2 the spectrum of the host galaxy HS1035+4758 is shown, in which typical HII-galaxy narrow emission lines are seen: H 4861, [OIII] 4959,5007, H 6562, [NII] 6548,6584 and [SII] 6716,6731 ?. ... The spectral evolution of SN 1998bv is illustrated in Fig. ... The change of the spectrum between April 6 and 19 with clear reddening shortward of H during these 2 weeks indicates seemingly that the 1st spectrum was observed in the period between the 20th and 30th days after the peak of the light curve...

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• The very metal-poor local dwarf galaxies
• H I and dynamical mass
• Old "Structure" publications

... We consider the astrophysical evolution of the Galaxy over large time scales, from early stages (an age of ~10 8 yrs) to the end of traditional stellar evolution (~10 11 yrs). ... In the model considered, the basic stages of Galactic evolution are as follows. ... Essentially all other basic parameters of the Galaxy vary little. ... The final "stellar epoch" in the life of the Galaxy is completed ~10 13 yrs after its formation, when the evolution of the least massive stars comes to an end. ...

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• Publications of Dmitri Wiebe
• Self-Consistent Model
• chemazh

... Gomez, J. C., Athanassoula, L., Fuentes, O., & Bosma, A. 2003, in ASP Conf. ... In this work we present Evolution Strategies (ES) as an efficient method to approximate the initial conditions of the main interacting group of three galaxies in M81. ... In this first attempt we use non-self-gravitating simulations to approximate the initial conditions; even with that restriction our method reproduces the density distribution of the three galaxies with great precision. ...

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• ADASS 2002 Conference Proceedings
• Improvements in Filter Design for Removing Galactic ``Cirrus'' from IRAS Images
• Using Massively Parallel Processing of a NLTE Spectrum Synthetic Code and an

... Viewing the Universe with Infrared Eyes: The Spitzer Space Telescope . Dr Giovanni Fazio . ... He then lead the development of large balloon-borne telescopes for far-infrared astronomical observations above the atmosphere, as Principal Investigator for the 1-Meter Balloon-Borne Far-Infrared Telescope and also the first infrared astronomical telescope to fly on the Spacelab II flight of the Space Shuttle. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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home education > activities . ... Quick math activity that asks students to calculate scale models of a binary star system with a black hole in it. [h] . ... Students use a radiometer and a light bulb with a dimmer switch to make connections between the temperature, color, and radiation output of a star. ... This demonstration, similar to the above, from the Exploratorium Snack-book of science activities, lets students demonstrate how molecules scatter light and change the colors of the beam. [m,h] . ...

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• Astronomical Society
• ASP: A Good Definition of the Word "Planet": Mission Impossible?
• ASP: Project ASTRO History & Evolution

... Behemoth black hole found in an unlikely place . ... Texas-sized computer finds most massive black hole in galaxy M87 . ... Astronomers Karl Gebhardt from The University of Texas at Austin and Jens Thomas from the Max Planck Institute for Extraterrestrial Physics have used new computer modeling techniques to discover that the black hole at the heart of M87, one of the largest nearby giant galaxies, is two to three times more massive than previously thought. ... Giant galaxy M87 finally sized up . ...

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• GRBs result of stellar swaps | Astronomy.com
• Cosmic evolution in a computer | Astronomy.com
• Astronomers discover close-knit pairs of massive black holes | Astronomy.com

... the radiative transfer equation (RTE) for the randomly-irregular magnetized plasma has been derived on the base of general grounds of the multiple scattering theory . ... Solutions of several absolute tasks of the scattering theory have been obtained (on the optical depth of the ionospheric plasma layer, on the value of radio wave anomalous attenuation, on anomalous refraction, on the backscattered signal intensity for the source being placed within a plasma layer). ...

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• Vladimir Marsakov Publication List
• T.Borkova, V.Marsakov, Distant globular clusters with anomalously small masses
• Vladimir Marsakov Abstracts

... Stars . ... Cepheid variable stars have been known since the 18th century. ... Regularly brightening to a peak over days, weeks or months before fading these variable stars were remarkable curiosities to astronomers in past centuries.€а The term Cepheid is taken from the star Delta Cephei in the constellation of Cepheus, which was identified as variable€а in 1784 by the teenaged prodigy John Goodricke (1764-96). ... Tweets that mention Cepheids: Inconstant Stars which break the rules | ...

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... Team . ... V.V.Sokolov "The gamma-ray bursts, core-collapse supernovae and global star forming rate at large redshifts" . ... I.V.Sokolov, A.S.Moskvitin, Eda Sonbas, O.V.Verkhodanov, O.P.Zhelenkova "A galaxy cluster in the GRB 021004 field" . ... The monitoring of GRB afterglows and the study of their host galaxies with the SAO RAS 6-m telescope from 1997". ... A.S.Moskvitin, T.A.Fatkhullin, V.V.Sokolov and V.N.Komarova, "Spectral and photometric monitoring of CCSNe at SAO RAS" . ...

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• Results scientific researchs 8
• Results scientific researchs 24
• About laboratory

THE STAR FORMATION NEWSLETTER An electronic publication dedicated to early stel lar/planetary evolution and molecular clouds No. 256 -- 10 April 2014 Editor: Bo Reipurth (reipurth@ifa.hawaii.edu) A: Steve and I had acquired experience in the numerical calculations of accreting massive stars for our pro ject on primordial protostars. ... Part of our group had developed a keen interest in the search for young massive stars, but it was difficult at the time to select the appropriate sources. ...

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• APOD: October 2, 1999 - Phi Persei: Double Star
• Formation and Early Evolution of Intermediate-Mass Stars
• Arcetri Star-formation Group Research Topics

The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

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• Methods and results of radio cosmology. Plan.
• Astronomical Schools
• Radio galaxies

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... ISS Russian Segment . Steps of ISS Assembly . ... Five new devices of the total mass of ~42 kg (instead of 6 devices of the total mass of ~101 kg) are installed in the guidance, navigation and control system of the new series vehicle. ... liquid thermostatting of GN OC devices is provided by installation of three cold plates in the vehicle instrument module (IM); . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

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... Liyong Liu (NAOC) . Site testing on seeing conditions of the astronomical observatories over China are briefly reviewed, including Xionglong station of NAOC, Gaomeigu station of Yunnan Observatory, Delingha station of Purple Mountain Observatory. ... PDF [3.0€аMB] October 8, 09:55 10:20 . ... In this paper, we will review the site survey activities in the past years, and present the site-testing results on the Oma site, including cloud cover, seeing, water vapor, transparency and sky brightness. ...

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• Results of ELT site testing programs - I
• Results of ELT site testing programs - II
• General information

... astro-ph . ... We present the goals and preliminary results of an unbiased, near-infrared, narrow-band imaging survey of the First Galactic Quadrant (10deg<l<65deg ; -1.3deg<b<+1.3deg). ... We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. ... Through Doppler imaging we want to study the spot evolution of the star and in particular compare this with previous results showing a cyclic spot behaviour and persistent active longitudes. ...

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APAO is a relatively new Olympiad which was founded in the spring 2005 as an international regional programme in line with the International Astronomy Olympiad. The 11 th Asian-Pacific Astronomy Olympiad (XI APAO) took place in November 2015 in Ashulia , Savar, North-West suburban area in Dhaka province , Central part of Bangladesh ). ... Theoretical and Practical rounds were held in Daffodil International University auditoriums. ... For the best result in all the rounds . ...

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• XIV International Astronomy Olympiad: Summaries. Results
• XIII International Astronomy Olympiad: Summaries. Results
• The X Asian-Pacific Astronomy Olympiad: Results

Central Bodies Masses of Selected Globular Clusters N.A.Shakht, A.A.Kiselev, Yu.N.Gnedin and E.A.Grosheva. The Main Astronomical (Pulkovo) Observatory RAS 47 Tuc ­NGC 104 RA 00 24 .1 Dec -72° 04 .9 Size = 30.9 mvis + 4. 0 m D from = 12,1 kpc, h m Cen - NGC 5139 NGC 6397 (Ara) RA 17 h40.m7 Dec -53o 40'.4 Size = 31',0 mvis + 5,3m D from =2.3 kpc RA 13h 26m .8 Dec -47° 28 6 Size = 36.3 m vis +3. 7 m D from =15.8 ±1.1 kpc, 12109 years, Age: 10109 years, (13.4 ± 0.8)109 years. ...

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• http://www.puldb.ru/jenam_2011/PUB_JENAM_2011/shakht_2.pdf
• http://www.puldb.ru/jenam_2011/PUB_JENAM_2011/Orlov_et_al_zhr.pdf
• http://www.puldb.ru/laza_gao/FOR_page_11/naroo_2012.pdf

Yu.V.Milanova, A.F.Kholtygin . Evolution of Elemental Abundances in Planetary Nebulae . Astronomy Letters, 32 , 557-565 ( 2006 ) . ... The theoretical dependences of the C and N abundances on Mini have been found to correspond to the observed ones. ... We have derived the relation between the abundances of the elements under consideration in planetary nebulae and the masses of their central stars. This relation is used to construct the mass function for the nuclei of planetary nebulae. ...

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• Vladimir P. Reshetnikov's Home Page
• Астрономия в Санкт-Петербургском университете |
• Model realization and some results

Добро пожаловать, Гость . ... В теме В разделе По форуму . Общероссийская неделя "Астрономия на тротуаре" - 15-17 апреля . ... Практическая астрономия ? Телескопостроение, оптика (Модераторы: I.A.R. , Ivan7enych ) ? обзор "Evolution of astronomical eyepieces" . предыдущая тема следующая тема . ... 0 Пользователей и 1 Гость просматривают эту тему. Гость . ... Если кому интересно, ищите здесь (придется зарегистрироваться на groups.yahoo.com): . ...

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