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21. http://www.ipa.nw.ru/conference/2002/sovet/PS/SOKOL_L.PS
... Many massive planets contrary to Jupiter have large eccentricities of orbits. ... Another problem is to study the conditions and boundaries of stable, regular motions of small mass planet in systems having `Jupiter' with large orbital eccentricity as well as properties of regular, stable, and irregular, chaotic motions. ... The regular eccentricity evolution described above demonstrates that stable quasi--circular orbits of small planet are unusual. ...
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Ссылки http://www.ipa.nw.ru/conference/2002/sovet/PS/SOKOL_L.PS -- 32.2 Кб -- 19.08.2002
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22. New LBV Star Discovered in the Galaxy
... Luminous blue variable (LBV) stars are the most massive stars with 40-120 solar masses, which are passing the short stage of evolution losing their hydrogen envelopes before exploding as Supernovae. These are extremely rare objects, only about a dozen of the most massive LBVs are known in the Galaxy. ... In the spectral observations of stars with infrared circular nebulae, found in the Spitzer survey (24 microns), a new LBV star in the Galaxy was discovered. It was named MN112. ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2010/LBV-3/ -- 4.4 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2010/LBV-3/ -- 4.4 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2010/LBV-3/ -- 4.4 Кб -- 02.10.2012
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23. http://jet.sao.ru/jet/~goray/838/v838ecl.htm
... V838 Mon is a member of a new class of eruptive variables which appear as a peculiar novae having late K-M type spectra in their outburst. Before its outburst, it was a wide binary system of B3V type stars. ... The B3V companion was seen in the outburst in the UV spectrum taken with HST (Rauch et al., ... In the latest spectra, the light of B3V companion was predominating in the short-wave photometric bands. ... CCD blue frames of V838 Mon before the eclipse (left) and in the eclipse (right). ...
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Ссылки http://jet.sao.ru/jet/~goray/838/v838ecl.htm -- 7.3 Кб -- 08.01.2007
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24. Science Innovations
. Сайт временно не работает.
25. Seminars
... в конференц-зале ГАИШ в 14 00 . ... Секретарь семинара М.К. Абубекеров . ... Липунов В.М. (ГАИШ МГУ) . ... Бескин В.С. (ФИАН РАН) . сопредседатель . ... Митрофанов И.Г. (ИКИ РАН) . ... Постнов К.А. (ГАИШ МГУ) . ... Курт В.Г. (АКЦ ФИАН) . ... Прохоров М.Е. (ГАИШ МГУ) . ... Имеется огромная потребность в обмене идеями и информацией сильно разделившихся в последние годы астрономических центров - ГАИШ, ФИАН (теор отдел), ИТЭФ, АКЦ ФИАН, Институт Астрономии, ИКИ, ИПМ, Институт Физпроблем, ИЯИ .. ...
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Ссылки http://xray.sai.msu.ru/sciwork/seminars.html -- 7.7 Кб -- 24.05.2010
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26. Cepheid Variables
... CEPHEID VARIABLE STARS: A Cepheid variable or Cepheid is a member of a particular class of very luminous, massive variable stars with pulsation periods of 1-70 days. ... The relationship is calibrated using data collected from Cepheids whose distances are determined by other means. ... Browse through the 68 CCD fits images he sent you, using ds9 and locate the Cepheid variable. ... Image credits: ESA - "http://sci.esa.int/science-e-media/img/20/cepheid-variables.jpg" . ...
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Ссылки http://www.mso.anu.edu.au/~jerjen/researchprojects/cepheids/cepheids.html -- 8.3 Кб -- 02.10.2012
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27. http://www.atnf.csiro.au/whats_on/workshops/mm_science2001/talks/Rudnitskij.pdf
Molecular Masers in Variable Stars Georgij Rudnitskij Sternberg Astronomical Institute, Moscow State University, Russia Millimetre Science with the Upgraded Australia Telescope 1 Late- type Variables · Red giant stars, M ~ 1 to a few M¤, L ~ a few 103 L¤, · Brightness varies at timescales of tens and hundreds of days, due to stellar pulsations. ... 2001) H2O line profiles Millimetre Science with the Upgraded Australia Telescope 8 RS Virginis , H2O, 1981- 2000 ( Lekht et al. ...
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Ссылки http://www.atnf.csiro.au/whats_on/workshops/mm_science2001/talks/Rudnitskij.pdf -- 500.7 Кб -- 23.04.2002
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28. http://www.badastronomy.com/pr/testimonials/speakinglist.doc
... Scientific Venues American Association for the Advancement of Science meeting American Astronomical Society meeting American Association of Physics Teachers meeting American Association of Variable Star Observers meeting .Astronomy Conference. ... Worth, TX University of Nebraska, Lincoln, NE Yale University, CT Conventions/Special Interest Meetings/Other (James Randi's) "The Amaz!ng Meeting" (2003 - 2009), Las Vegas, NV, Ft. ... Diablo Astronomical Society, Concord, CA Mt. ...
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Ссылки http://www.badastronomy.com/pr/testimonials/speakinglist.doc -- 41.5 Кб -- 05.03.2011
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29. Astrophysics Group COAST Astronomical Results
... Astrophysics Group . ... COAST . COAST Astronomical Results . ... Surface Imaging of Betelgeuse . ... This page highlights some astronomical results obtained with COAST over the years. These are listed in chronological order (most recent first). ... Measurements of cyclic variations in the angular diameter of Chi Cygni . ... The first infrared image from an aperture synthesis array . ... The images of Betelgeuse below were reconstructed from COAST data taken in early 2004. ...
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Ссылки http://www.mrao.cam.ac.uk/outreach/radio-telescopes/coast/coast-astronomical-results/ -- 22.3 Кб -- 10.04.2016
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30. Arecibo Radar Discovers Triple Near-Earth Asteroid
Image credit: Michael Nolan, Arecibo Observatory. These radar images of near-Earth asteroid 2001 SN263 were obtained on 2008 Feb 12 and 13. ... Image from Feb 12 . ... First near-Earth triple asteroid discovered by Arecibo Observatory . ... was discovered this week by astronomers at the sensitive radar telescope at Cornell University?s Arecibo Observatory in Puerto Rico. ... For example, Arecibo has discovered more than half of the near-Earth binary asteroid systems discovered since 1999. ...
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Ссылки http://www.naic.edu/~pradar/asteroids/2001SN263/ -- 7.7 Кб -- 23.02.2008
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31. New Satellites of Saturn
New Satellites of Saturn . On July 26, 1995, Amanda Bosh of Lowell Observatory announced the discovery of at least two and perhaps four new satellites of Saturn . The discovery was based upon images taken by the Hubble Space Telescope on May 22, 1995, when Saturn's rings were tilted edge-on to the Earth . ... The two satellites S/1995 S1 and S2 lie inside Saturn's thin, eccentric "F" ring . ... The fourth satellite S/1995 S4 is 6,000 kilometers (3,700 miles) beyond the F ring. ... S/1995 S 3 . ...
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Ссылки http://www.iki.rssi.ru/solar/eng/satnew.htm -- 5.8 Кб -- 15.10.1997
[ Сохраненная копия ] Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/satnew.htm -- 6.7 Кб -- 15.03.1998
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[ Сохраненная копия ] Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/satnew.htm -- 6.7 Кб -- 15.03.1998
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32. Science - Page 2
... Dept. for Astrometry & Space Geodynamics . ... Dept. for Physics of Stars&Galaxies . ... Dept. for Physics of Planetary Systems . ... Science . ... All Pages . ... Research of the stars with planets which pass apparent star disk (transiting exoplanets). The transit method based on a detection star brightness decrease during a passing of planet in front of its disk. Observed brightness system decries when planet pass star disk and its volume depend of the relative sizes star and planet. ...
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Ссылки http://www.mao.kiev.ua/index.php/en/instruments/internet-telescope?showall=&start=1 -- 18.9 Кб -- 11.04.2016
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33. Modelling Spectro-photometric Characteristics of Eclipsing Binaries
... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...
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Ссылки http://www.stecf.org/conferences/adass/adassVII/polubekg.html -- 15.8 Кб -- 12.06.2006
[ Сохраненная копия ] Ссылки http://www.adass.org/adass/proceedings/adass97/polubekg.html -- 15.8 Кб -- 15.05.1998
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[ Сохраненная копия ] Ссылки http://www.adass.org/adass/proceedings/adass97/polubekg.html -- 15.8 Кб -- 15.05.1998
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34. "Structure" publications in 2008 year
Our publications in 2008 year Ekta; Chengalur, Jayaram N.; Pustilnik, S. A. Monthly Notices of the Royal Astronomical Society, Volume 391, Issue 2, pp. ... Astronomy Letters, Volume 34, Issue 7, pp.457-467 (07/2008) . Pustilnik, S. A.; Tepliakova, A. L.; Kniazev, A. Y.; Burenkov, A. N. Monthly Notices of the Royal Astronomical Society: Letters, Volume 388, Issue 1, pp. ... Kniazev, A. Y.; Pustilnik, S. A.; Zucker, D. B. Monthly Notices of the Royal Astronomical Society, Volume 384, Issue 3, pp. ...
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Ссылки http://www.sao.ru/precise/Laboratory/Publications/2008_pub.html -- 3.5 Кб -- 07.07.2009
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35. http://www.izmiran.rssi.ru/~obridko/papers/2004IAUS_223_371B.pdf
... It is found that the correlation coefficients between these two parameters calculated separately inside and outside the sunspot formation zone ±30 have cyclic variation and occur in anti-phase. This suggests different mechanisms of formation of the corona in the fields of small, medium, and large scales. ... The relationship between the coronal green line brightness (CGLB) and the magnetic field strength (MFS) has been investigated by constructing the corresponding synoptic maps for the 1977-2001. ...
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Ссылки http://www.izmiran.rssi.ru/~obridko/papers/2004IAUS_223_371B.pdf -- 73.7 Кб -- 17.11.2015
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36. http://www.issp.ac.ru/iao/2015/booklet/b10_ia15_p_en_a.pdf
... A star was observed at different zenith distances during one night at the Engelgardt's Astronomical Observatory in the program of atmospheric extinction study at blue. ... The determination of the star's brightness was performed with the method of photon counting. ... Variable star. ... The brightness of the variable star was measured occasionally during the other nights, and moments of maximal values of brightness (15.59m) were received on nights 25, the 2nd table. ... JD 2452805. ...
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Ссылки http://www.issp.ac.ru/iao/2015/booklet/b10_ia15_p_en_a.pdf -- 173.2 Кб -- 03.12.2015
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37. http://hea.iki.rssi.ru/integral06/papers/E37_Hudec01-16Feb07_17:08:21.pdf
IDENTIFICATION OF INTEGRAL SOURCES WITH ASTRONOMICAL ARCHIVAL PLATES (1,2) (1,2) RenИ Hudec (1) , Filip Munz , Petr KubАnek( 1,2) Astronomical Institute, Academy of Sciences of the Czech Republic, CZ-251 65 Ond ejov, Czech Republic E-mail:rhudec@asu.cas.cz (2) INTEGRAL ISDC, Versoix, Switzerland ABSTRACT The ESA INTEGRAL satellite (International Gamma Ray Laboratory) launched in October 2002 continues to deliver valuable data about the gamma-ray sky. ... LEIDEN/JOHANNESBURG F.A. PLATES 8. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/E37_Hudec01-16Feb07_17:08:21.pdf -- 742.0 Кб -- 16.02.2007
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39. Vladislav V. Shevchenko
... Shevchenko Vladislav Vladimirovich . ... Position: Head of Department of Lunar and Planetary Research, Sternberg State Astronomical Institute, Moscow University, Doctor of Physics and Mathematics. ... L. Johnson Space Center - Lunar and Planetary Institute. ... Sternberg State Astronomical Institute, Moscow University, Universitetsky 13, Moscow, 119899 , Russia, . ... V.I.Chikmachev, S.G.Pugacheva and V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Moscow, chik@sai.msu.ru ...
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Ссылки http://selena.sai.msu.ru/Shev/ShevE.htm -- 13.4 Кб -- 20.04.2015
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40. Pulkovo Observatory
. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.
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