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21. http://www.atnf.csiro.au/people/plintel/groups/lsse/articles/abstracts/9201.html
OH/IR stars as the progenitors of planetary nebulae P. te Lintel Hekkert and A.A. Zijlstra Based on a new sample of (IRAS based) OH/IR stars, and the catalogue of planetary nebulae compiled by Acker (1983), we study the relation between these two groups of objects, in terms of the kinematics and the Galactic distribution. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/plintel/groups/lsse/articles/abstracts/9201.html -- 3.1 Кб -- 28.06.2010
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22. SN 1989B Light Curve Analysis.
SN 1989B Light Curve Analysis. ... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... The observations were inserted against the V magnitude templete of BL, CCD photometric data, (Wells et. al, (1994) and a color trend (B-V) histogram of the mean type Ia SN (BL)(nutemp.gif). Key Words: Amateur Observations, Supernova, Magnitude Estimates, 1989B . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/analysis.htm -- 5.1 Кб -- 02.02.2012
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23. Towards a Truly Unified Model of AGN
... Towards a Truly Unified Model of AGN . ... The Unified Model holds that the aspect-dependent effects primarily determine the nature of the active galactic nucleus that we observe. ... The full postscript file can be obtained here: . The PASA Latex file can be obtained here: . The postscript file of Fig 1 can be obtained here: . ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~mad/unified.html -- 6.8 Кб -- 09.04.2016
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24. Six-Centimeter Radar Observations of 4179 Toutatis
... Old World First Asteroid Radar Echo. ... It testifies that 4179 Toutatis is a double object like asteroid 4769 Castalia. ... Interference of Radar Echo from the Binary Asteroid 4179 Toutatis. ... An analysis of the 6-cm radar data revealed quasi-harmonic oscillation of the echo’s “central” Doppler frequency with a period of about 14 sec and a deviation of about (0.7*B) Hz, where B is the echo bandwidth, which for 4179 Toutatis was equal to 2.1 Hz and 1.9 Hz for 1992 Dec 8 and 9, respectively. ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/html/ra&sr/sr/4179-Toutatis/index.html -- 11.9 Кб -- 02.12.2002
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25. Keywords_7
. Determination of UTO from lunar laser ranging data analysis . E. Yu. Aleshkina . Institute of Applied Astronomy, St. Petersburg, Russia Abstract: . No abstract Key words: . Very Long Baseline Interferometry (VLBI), celestial mechanics, UTO, lunar laser ranging data analysis.
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/EDITION/transaction/transaction_ann08/7.htm -- 3.0 Кб -- 02.10.2012
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26. Vladimir V. Busarev
... V.V. Busarev, Sternberg State Astronomical Institute, Moscow University, . ... V. V. Busarev1, M. N. Taran2, V. I. Fel’dman3 and V. S. Rusakov41 Lunar and Planetary Department, Sternberg State Astronomical Institute, Moscow State University, 119992 Moscow, Universitetskij pr., ... 1 Sternberg State Astronomical Institute, Moscow University, Universitetskij pr., ... V. V. BUSAREV, Sternberg State Astronomical Institute, Moscow University, Russian Federation (RF) (E-mail: busarev@sai.msu.ru); . ...
[ Сохраненная копия ]  Ссылки http://selena.sai.msu.ru/Bus/BusE.htm -- 16.1 Кб -- 20.04.2015
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27. astro-ph authors/title/abstract search for 'galaxy environment' all years
Title: A Dark-Matter Spike at the Galactic Center? Authors: Piero Ullio , HongSheng Zhao , Marc Kamionkowski . ... Title: The Galaxy Environment of Quasars in the Clowes-Campusano Large Quasar Group at z~1.3 . ... Title: The Galaxy Environment of a Quasar at z=1.226: A Possible Cluster Merger . ... 16 matches for the search pattern galaxy environment . The URL for this page is: http://xxx.itep.ru/find/astro-ph/1/galaxy+environment/0/1/0/past,all/0/0 www-admin@xxx.lanl.gov ...
[ Сохраненная копия ]  Ссылки http://sed.sao.ru/lit/gal_envir.html -- 16.6 Кб -- 15.07.2001
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28. http://www.izmiran.rssi.ru/~obridko/papers/320.pdf
... Figure 1a illustrates the summary diagram (2 log L, log S ) based on the field intensity contour lines for 7 active regions plotted at 200 G steps in the range of 2200­400 G. One can see that the relationship under discussion is well represented by two straight lines, one corresponding to the log S range from 2 to 7.2 and another, from 7.2 to 9. ... Then, we plotted 2 log L versus log S for all field lines of a given intensity, no matter which sunspot or sunspot group they belonged to. ...
[ Текст ]  Ссылки http://www.izmiran.rssi.ru/~obridko/papers/320.pdf -- 77.9 Кб -- 07.04.2011
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29. University Satellites and Space Science Education '2006
University Satellites and . Space Science Education . ... It is necessary to select a topic interesting from scientific point of view and simple enough to allow students understand and participate in all stages of experiment from measurements via data analysis to physical inference. ... Solar modulation effects and physical characteristics and analysis of the major solar events are possible only by joining data from space-born and surface particle and radiation detectors. ...
[ Сохраненная копия ]  Ссылки http://cosmos.msu.ru/universat2006/main.php?sec=reg&step=aview&id=1182&aid=921 -- 10.1 Кб -- 21.12.2007
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30. Space Research Institute (IKI) Seminar
... Abstract . ... I.V. Holin (Space Research Institute of RAS (IKI)) . ... Space Research Institute of Russian Academy of Science (IKI)) . ... Skulachev, Dmitri P. (Space Research Institute of RAS (IKI)) . ... Elena Gavryuseva (National Institute of Astrophysics and Space Physics, Florence , Italy and Institute of Nuclear Research of RAN) . ... Dmitri Vainchtein (Space Research Institute of Russian Academy of Sciences) . ... Elena Surovyatkina (Space Research Institute of Russian Academy of Sciences) ....
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/galeev/english/past2008.htm -- 58.2 Кб -- 14.03.2011
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/galeev/english/past2008.htm -- 58.2 Кб -- 14.03.2011
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31. ADS Abstract Service Results
... Study of Mg-Fe-silicate glasses of variable composition. ... With the new data, the astrophysical discussion started in Paper I was continued and focussed on the comparison of the olivine glass data with IRAS LRS spectra of O-rich circumstellar envelopes around Mira stars. ... The new olivine glasses point to the in