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Ïîêàçàíû äîêóìåíòû, ñîäåðæàùèå ôðàãìåíòû òåêñòà èç äîêóìåíòà
http://www.sai.msu.su/mirrors/isn/sn2000/sn2000dx.html.

21. Supernova spotted by Irish astronomer | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... As example you have only to look at the recent discovery of a supernova by Irish astronomer David Grennan . ... The last confirmed supernova in the Milky Way to be observed was in 1604 (known to history as Kepler ?s Star; it was bright enough to be seen in the daytime sky). ˆà Ever since then all supernovae examined by astronomers have been denizens of other galaxies. ... Tweets that mention Supernova spotted by Irish astronomer -- Topsy.com . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.armaghplanet.com/blog/supernova-spotted-by-irish-astronomer.html -- 43.4 Êá -- 09.04.2016
Ïîõîæèå äîêóìåíòû

22. Ceresò?? bright spots show unexpected changes | Astronomy.com
... Ceresò?? bright spots show unexpected changes . ... CERES | ... Observations made using the HARPS spectrograph at the European Southern Observatory s (ESO) La Silla Observatory in Chile have revealed unexpected changes in the bright spots on the dwarf planet Ceres. Although Ceres appears as little more than a point of light from Earth, careful study of its light shows not only the changes expected as Ceres rotates, but also that the spots brighten during the day and also show other variations. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.astronomy.com/news/2016/03/ceres-bright-spots-show-unexpected-changes -- 70.3 Êá -- 10.04.2016
Ïîõîæèå äîêóìåíòû

23. http://www.asc.rssi.ru/RadioAstron/meetings/telecon/nov16_2011.pdf
... N. Kardashev and M. Popov informed the participants on the current IOC results. ... Kovalev). ... Agenda of the RadioAstron teleconference November 16, 2011 Corrections to the Agenda 1 2 3 4 5 6 IOC status and results Single Dish observation with RA VLBA observations to find best fringe search candidates Fringe search plan Early science program plan Tracking stations outside Russia N.Kardashev N. Kardashev / M.Popov V. Kostenko E.Fomalont M.Popov Y.Y. Kovalev / M.Popov /A.Alakoz ...
[ Òåêñò ]  Ññûëêè http://www.asc.rssi.ru/RadioAstron/meetings/telecon/nov16_2011.pdf -- 24.6 Êá -- 13.12.2011
Ïîõîæèå äîêóìåíòû

24. V.Shergin's Home Page
... Description(Russian): [ HTML ] [ PDF ] . ... 2002 : source L A T E X and export to [ HTML ], [ PDF ], [ PS ], [ OpenOffice ], [ MSWord ] . 2003 : source L A T E X and export to [ HTML ], [ PDF ], [ PS ], [ OpenOffice ], [ MSWord ] . 2004 : source L A T E X and export to [ HTML ], [ PDF ], [ PS ], [ StarOffice ], [ MSWord ] . 2005 : source L A T E X and export to [ HTML ], [ PDF ], [ PS ], [ StarOffice ], [ MSWord ] . ... 2014 : source HTML and export to [ PDF ], [ MSWord ], [ ODT ] . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://mavr.sao.ru/hq/vsher/ -- 21.4 Êá -- 09.04.2016
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sao.ru/hq/vsher/ -- 21.4 Êá -- 09.04.2016
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://jet.sao.ru/hq/vsher/ -- 21.4 Êá -- 09.04.2016
Ïîõîæèå äîêóìåíòû

25. February 2002 APT Meeting
... APT Activities and Science Results 3. ... APT Secretary Philip Edwards (ISAS) reviewed the aims of the APT (http://www.vsop.isas.ac.jp/apt/DefinitionAndAims.html). ... The Australia Telescope Compact Array, and Ceduna, Hartebeesthoek, Kashima, Mopra, Parkes, and Shanghai telescopes of the Asia-Pacific Telescope participated in these observations. ... In the absence of Tetsuo Sasao, Philip Edwards briefly described results of the APT 22 GHz observations conducted from October 1st to 5th, 1997. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.vsop.isas.ac.jp/apt/meetings/APTfeb2002summary.html -- 5.3 Êá -- 23.10.2002
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>22) - www.vsop.isas.ac.jp/ )

26. The RATAN SNRs Survey
... 81Trushkin+ The results of the multi-frequency radio observations of fourteen supernova remnants (SNRs) made with the RATAN-600 radio telescope in 1985 are reported. Flux densities of these SNRs are measured at least at two wavelengths: 31.3 and 7.6 cm. The radio spectra of some SNRs are precised. ... The radio sources detected inside or near the SNRs with the flux densities measured in the most sensitive 7.6-cm radiometer. The spectra of some point sources are discussed. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sao.ru/cats/doc/SNR_Trushkin2.html -- 2.6 Êá -- 18.03.2015
Ïîõîæèå äîêóìåíòû

27. http://observ.pereplet.ru/IAUC8520.html
... SUPERNOVAE 2005bv AND 2005bw . ... IAUC 8515; 0.60-m automated supernova patrol telescope ). ... Offset 2005bv š Apr . ... IAUC 7178). SUPERNOVAE 2005bf AND 2005bq . ... IAUC 8515), obtained in the course of the Carnegie Supernova Project on Apr. ... IAUC 8507, 8509) is undergoing an unusual photometric behavior, brightening from u' = 18.69 on Apr. 7 to u' = 17.90 on Apr. 13, and declining to u' = 18.61 on Apr. 21, after which it has been re- brightening (reaching u' = 17.92 on Apr. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://observ.pereplet.ru/IAUC8520.html -- 24.1 Êá -- 01.10.2012
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28. http://www.izmiran.rssi.ru/services/saf/archive/en/2013/obzor20131216.en.txt
Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 09 - 15.12.2013, Forecast on 16 - 23.12.2013, Carrington Rotation 2144, 2145 ( 21,73.11; 19,05.2013) SUNSPOT-FORMING ACTIVITY OF THE SUN AFTER 10.12 REMAINED AT HIGH LEVEL. ... NEXT WEEK IS EXPECTED THE HIGH AND AVERAGE LEVEL OF SUNSPOT ACTIVI- TY. ... DURING THE REPORTING PERIOD 3 GEOFFCTIVE (SMALL RATE) EJECTA OF SOLAR FILAMENT, WHICH IS ACCOMPANIED BY CME TYPE "PARTIAL HALO II" WAS OBSERVED. ... Class E(1-8A) AR RII/IV CME X / opt. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.izmiran.rssi.ru/services/saf/archive/en/2013/obzor20131216.en.txt -- 5.2 Êá -- 16.12.2013
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29. So Where Is Mars Now? - an Astronomy Net Observation_reports Forum Message
Astronomy Discussion Forums . Forums: . ... Discussion Forums . ... So Where Is Mars Now? Forum List | ... Post Message | ... Posted by Moazzam on September 4, 2003 20:09:09 UTC . ... Login to Post . ... www.astronomy.net . About Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.astronomy.net/forums/observation_reports/messages/264.shtml -- 13.5 Êá -- 09.04.2016
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30. 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.
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.gao.spb.ru/ -- 4.5 Êá -- 06.04.2009
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31. TAP 26
Next: P1724 Up: Specific Stars Previous: Specific Stars . ... They reported a 2.5 day rotation period for this star which they confirmed with their 1995 results (Bouvier et al . 1995). ... only averaged one measurement per night, they were not sensitive to periods of < 2 days. ... TAP 26 was monitored from MTSB on 15 nights. ... If one confines the period search range for the MTSB data to be greater than one day, the results are nearly identical to those for the data presented by Bouvier et al . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://hea-www.harvard.edu/~swolk/thesis/results/node2.html -- 5.4 Êá -- 02.10.2012
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32. Kholtygin et al., Magn. Field Conf., August 2003 (2004)
Kholtygin A., Brown J., Fabrika S., Surkov A. Magnetic field connected fast line profile variability in spectra of bright O supergiants . ... Conference, held in the Special Astrophysical Observatory of the Russian AS, August 27-31, 2003, Eds.: Yu. ... Results of a study of fast line profile variability ( lpv ) in spectra of selected bright O-stars are reported. ... In the context of testing the MCWS model a program of searching for weak magnetic fields in bright O and early B stars is outlined. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.astro.spbu.ru/staff/afk/Papers/2004/MgnFld2004abstr.html -- 2.4 Êá -- 19.11.2010
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33. Lecture Series 2010-2011 ? ?Top Ten Discoveries of the Phoenix Misson to Mars?
Lectures . ... Home Lectures Lecture Series 2010-2011 Lecture Series 2010-2011 ? Top Ten Discoveries of the Phoenix Misson to Mars? by Suzanne Young . ... Lecture Series 2010-2011 . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... Amateur Astronomers Medal . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.aaa.org/lectures/lecture-series-2010-2011/lecture-series-2010-2011-top-ten-discoveries-of-the-phoenix-misson-to-mars-by-suzanne-young/ -- 101.0 Êá -- 10.04.2016
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34. ASP: Astronomy in the News
... In August 2009, amateur and professional astronomers reported that the bright star Epsilon Aurigae had begun to lose brightness for the first time in 27 years. ... Professional and amateur astronomers teamed up to monitor the eclipse and have announced that this critical phase ended around New Year s Day 2010. ... Even during the eclipse, the star is so bright that sensitive equipment in professional observatories can have trouble monitoring its brightness in the optical wavelengths. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.astrosociety.org/pubs/mercury/39_01/astronews.html -- 7.6 Êá -- 02.10.2012
Ïîõîæèå äîêóìåíòû

35. Science Innovations
. Ñàéò âðåìåííî íå ðàáîòàåò.
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sai.crimea.ua/ -- 1.9 Êá -- 17.05.2015
Ïîõîæèå äîêóìåíòû

36. Science with CXO
Next: Conclusion Up: No Title Previous: The Transmission Gratings . ... The potential of Chandra is illustrated in Figure which shows the official "first-light" image. ... Figure: The official CXO first light image - the supernova remnant CasA. Perhaps the neutron star - black hole connection and the utility of CXO are best illustrated by an early observation of the Crab Nebula and pulsar taken as part of the HETG calibration. ... Figure shows the zeroth-order image of the Crab Nebula. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://xray.sai.msu.ru/~polar/images/chandra/crete_astro-ph/node6.html -- 6.0 Êá -- 07.12.1999
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>571) - xray.sai.msu.ru/ )

37. http://www.wdcb.ru/stp/data/sudden.com/STORM2_1968_/storm2_fmt.txt
... Column Fmt Description ---------------------------------------------------------------------- 1 A1 Blank 2- 5 I4 Year (19__) 6- 8 A3 Blank 9-10 I2 Month 11-13 A3 Blank 14-15 I2 Day 16-17 A2 Blank 18-21 I4 Begin time 22-25 A4 Blank 26-27 I2 Number stations reporting an A event 28 A1 Letter A -- denotes very remarkable event observed 29-31 A3 Blank 32-33 I2 Number of stations reporting a B ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.wdcb.ru/stp/data/sudden.com/STORM2_1968_/storm2_fmt.txt -- 3.8 Êá -- 18.09.2015
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38. Detection of unique bright radio flare of X-ray binary
... The Galactic low-mass X-ray binary GS 2023+338 was discovered during the burst on May 22, 1989 with the Japanise satellite Ginga (aka Galaxy). The flux reached 17 crabs (this unit of flux measurement is an bright X-ray source, Crab Nebula) at 10-35 keV. ... No other radio telescope worldwide carried out multi-frequency measurements. ... Upon 14 days the radio flux fell below the detection level at the RATAN-600 in relation to the decrease of the X-ray flux. ...
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://www.sao.ru/Doc-en/SciNews/2016/Trushkin/ -- 8.4 Êá -- 10.04.2016
[ Ñîõðàíåííàÿ êîïèÿ ]  Ññûëêè http://mavr.sao.ru/Doc-en/SciNews/2016/Trushkin/ -- 8.4 Êá -- 10.04.2016
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>388) - mavr.sao.ru/ )

39. http://comet.sai.msu.ru/~gmr/poster_1.072.pdf
... OH, = 18 cm Nancay Radio Telescope, OH 18-cm line observations , since 1969 F, Jy 6 4 2 0 0 -1 -2 0 -1 -2 0 -2 -4 -6 30 40 50 1612 MHz I HU Pup August 5, 2009 1665 MHz 4 2 0 0.5 0.0 - 0.5 -1.0 -1.5 1.0 0.5 0.0 - 0.5 4 3 2 1 0 -1 1667 MHz I I 1.0 0.5 0.0 0.5 0.0 22-meter telescope, Pushchino Radio Astronomy Observatory H2O F, Jy 1.0 0.5 0.0 0.4 0.2 0.0 -0.2 -0.4 0.4 0.2 0.0 -0.2 -0.4 -0.6 0.6 0.4 0.2 0.0 -0.2 -0.4 -70 -60 -50 -40 -30 -20 -10 0 Mira-type star R Leo. ...
[ Òåêñò ]  Ññûëêè http://comet.sai.msu.ru/~gmr/poster_1.072.pdf -- 2627.4 Êá -- 16.06.2011
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>102) - comet.sai.msu.ru/ )

40. http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.ps.gz
... The Co­Addition Technique Applied to Images of Galaxy Cores W. W. Zeilinger Institut f˜ur Astronomie, University of Vienna, T˜urkenschanzstraúe 17, A­1180 Wien, Austria P. Crane, P. GrosbÜl and A. Renzini European Southern Observatory, Karl­Schwarzschild Straúe 2, D­85748 Garching, Germany Abstract. ... One may therefore take full advantage of the high resolution FOC images by co­adding them with (high signal­to­noise) ground­ based data. ... References Crane, P. et al. ...
[ Òåêñò ]  Ññûëêè http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.ps.gz -- 76.9 Êá -- 12.06.2006
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