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21. THE LABORATORY OF METEORITICS, VERNADSKY INSTITUTE, RAS
... About meteorites . ... About laboratory . ... Lunar sample collection . ... July 28 - August 1, 2003, Munster, Germany . Meteoritics and Planetary Science 38 (Supplement), A28. ... Meteoritics and Planetary Science 38 (Supplement), A30. LUNAR METEORITE DHOFAR 310: A POLYMICT BRECCIA WITH DEEP-SEATED LUNAR CRUSTAL MATERIAL . ... These studies present new evidence showing that NWA 011 is significantly different from HED meteorites. 34th Lunar and Planetary Science Conference . ...
[ Сохраненная копия ]  Ссылки http://www.meteorites.ru/publications-e.html -- 22.9 Кб -- 27.07.2011
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22. Transformation Groups 2007
The conference will be held at the Independent University of Moscow , located in the center of Moscow city. ... Steklov Mathematical Institute , . ... The conference " Transformation Groups " is aimed to review the development of Transformation Group Theory during last decades, to present the most bright recent achievements in this area, and to discuss the perspectives of further research. ... Dmitri N. Akhiezer (Institute of Information Transmission Problems, Moscow, Russia) . ... Russia) . ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/tg2007/main.html -- 11.7 Кб -- 02.01.2008
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23. http://hea-www.harvard.edu/~pgreen/SOC/9.html
... The Chandra COSMOS Survey 2. ... Evidence that Compton-thick and Compton-thin obscured AGN have two physically different origins on different scales are presented and the implications for surveys and AGN evolution are discussed. oral . Monday: Type I and II AGN, Absorption, XBONGs, Tuesday: AGN correlation functions, LSS, environments . ... Monday: X-ray luminosity functions and evolution, Tuesday: AGN correlation functions, LSS, environments . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~pgreen/SOC/9.html -- 6.4 Кб -- 01.10.2012
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24. G35.20-1.74 (Abstract)
... We present J(1.25 $\mic$), H(1.65 $\mic$), K(2.2 $\mic$), H$_2$(2.125 $\mic$) an d 11.2$\mic$ infrared images at sub-arcsec resolution of an area centered around the star forming region G~35.20--1.74. In J, H and K a cluster of early type stellar sources with infrared excess clearly stands out with respect to the background distribution and is associated with a diffuse K emission around an UC HII region (which is the brightest source at K). ... At 11.2$\mic$ six components are detected. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/g3520/abstract.html -- 3.6 Кб -- 11.09.2007
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25. http://www.naic.edu/vscience/schedule/2014Spring/DenevatagP2860.pdf
... Proposal Type: General Category: Observation Category: Time Requested this semester: Hours already used for this pro ject: Additional Hours required to complete pro ject: Minimum Useful Time: Expected Data Storage: Prop osal Title: ABSTRACT: Regular Pulsars Galactic 55.5 0 1.5 h over 500 GB Searching for Millisecond Pulsars in Low-Latitude Fermi Unidentified Sources We propose to search for pulsars in fourteen Fermi unidentified sources close to the Galactic plane (|b|<4 degrees). ...
[ Текст ]  Ссылки http://www.naic.edu/vscience/schedule/2014Spring/DenevatagP2860.pdf -- 61.6 Кб -- 06.09.2013
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26. Space Scientific and Education project of Lomonosov Moscow State University
Educational program of the project is intended for training of specialists in different fields of space physics, astronomy and the Earth sciences. ... Special space-physics lab exercises are intended for the students of the senior courses of the Institutions, specialized in the field of space engineering and space physics. Its main task is to teach them some methods of satellites scientific and engineering data processing. ...
[ Сохраненная копия ]  Ссылки http://cosmos.msu.ru/eng/eduprog.html -- 3.4 Кб -- 05.12.2005
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27. Home Page
XMM-Newton Science Analysis System . ... Meta Index . This task merges EPIC event lists or additional files (attitude, orbit) from two exposures (even from different observations and instruments), pointing in the same or an adjacent direction. Sky coordinates are (optionally) adjusted for attitude errors and then reprojected to a common reference point. The output files can be used by evselect and the higher level detection and time analysis tasks. ... Errors . ... Output Files . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/merge/index.html -- 4.2 Кб -- 01.07.2008
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28. Stellarium: TuiNodeEditable Class Reference
Stellarium 0.12.3 . ... Classes . ... TuiNodeEditable Class Reference abstract . pure virtual from which editables for different data types are derived. ... TuiNodeEditable (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... handleKey (int key) . ... TuiNode (const QString &text, TuiNode *parent=NULL, TuiNode *prev=NULL) . ... virtual QStringљ . ... virtual TuiNode *љ . ... virtual voidљ . ... home/aw/devel/stellarium/trunk/plugins/TextUserInterface/src/ TuiNodeEditable.hpp . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classTuiNodeEditable.html -- 19.8 Кб -- 28.02.2014
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29. Баллистический центр Института прикладной математики им. М.В.Келдыша РАН
... Институт прикладной математики им. М.В.Келдыша . БАЛЛИСТИЧЕСКИЙ ЦЕНТР . О Центре . ... Баллистический Центр Института прикладной математики им. М.В.Келдыша РАН . Баллистический центр (БЦ) ИПМ им. М.В. Келдыша создан по предложению С.П. Королева и М.В. Келдыша в 1965 году. На него были возложены работы по баллистико-навигационному обеспечению (БНО) управления полетом пилотируемых кораблей и автоматических космических аппаратов научного и народно-хозяйственного назначения. ...
[ Сохраненная копия ]  Ссылки http://www.kiam1.rssi.ru/ -- 4.2 Кб -- 02.02.2013
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30. 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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31. LPCBC: Abstract 2_32
... Comparative study of Tl-2201 single crystals with different temperatures of superconducting transition by means of specific heat method. Abstract: . The comparison studies of the specific heat of Tl-2201 single crystals with the different oxygen concentration have led to the conclusion that the doping by oxygen, resulting in lowering of T c and increasing of number of paramagnetic centers, leads to diminishing of antiferromagnetic correlations contribution to the specific heat. ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/lpcbc/ABST/2_32.html -- 2.2 Кб -- 24.12.1999
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32. http://www.atnf.csiro.au/people/Stuart.Weston/Posters/sweston-asa-asm-2012.pdf
... We present data for the additional lines after processing and baseline fitting H91, H92 within this HII region. Integrated line profiles for H90 (top left), H91 (top right) and H92 (bottom left) are all 16MHz bands with a resolution of 512. ... The radio recombination lines of hydrogen H90, H91, H92, helium He91 and carbon C91 were detected from OrionA, and H90, H91, H92 from M17 and NGC3603 at 8GHz. ... The recombination lines from left to right are H90 and H91. ...
[ Текст ]  Ссылки http://www.atnf.csiro.au/people/Stuart.Weston/Posters/sweston-asa-asm-2012.pdf -- 2077.0 Кб -- 09.07.2013
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33. Zeldovich-100 / International Conference / Moscow, Russia
Main Program Travel Where to go in Moscow Information . ... Conference Program . ... See also abstracts of the Talks and Posters . ... January 15 th : Call for abstracts . February 15 th : Deadline for abstract submission . March 15 th : Release of preliminary scientific program . March 15 th : Deadline for submission of information for visa support . ... International Conference: Cosmology and High Energy Astrophysics (Zeldovich-90) 20-24 Dec 2004, Moscow, Russia . Conference E-mail . ...
[ Сохраненная копия ]  Ссылки http://hea.iki.rssi.ru/zeldovich-100/index.php?p=program -- 10.3 Кб -- 10.04.2016
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34. Journal "Peremennye Zvezdy"
We inform the variable-star community that the publication of the "Peremennye Zvezdy" (Variable Stars) journal, founded by Prof. B.V. Kukarkin (1909 1977) in 1928, is planned to be resumed by November, 2005. Currently it is possible for us to publish "Peremennye Zvezdy" only as an electronic journal. ... The main journal will accept original scientific papers containing theoretical results as well as results based on detailed analysis of variable-star observations. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/varstars/msg/1208594 -- 9.4 Кб -- 14.10.2005
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35. ASP's 2010 Annual Meeting
... Annual Meeting . ... Scholarships for Cosmos . ... Download scholarship application instructions in pdf format. ... Scholarships will be provided after the meeting as reimbursement for document expenses incurred. ... While the deadline for scholarship application has now passed, there may be the possibility of additional funds from our generous meeting sponsors. You may submit a late application until June 30, 2010 and these will considered if funds become available. ... Cosmos Scholarships . ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/events/2010mtg/scholarships.html -- 22.0 Кб -- 05.09.2010
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36. Abstract 200
The total radiative power output from the hot outer layers of six late-type stars (of different spectral types and luminosity class) is derived via an emission measure technique. This analysis was based on observational data from the spectral range 100A to 3000A obtained as a result of three separate satellite missions, i.e. Hubble Space Telescope, International Ultraviolet Explorer and the Extreme Ultraviolet Explorer. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~ambn/abstract200.html -- 2.3 Кб -- 15.08.1996
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37. Optical Counterparts for 70,000 FIRST sources
... 2002ApJS.. 143.. ... Journal:* The Astrophysical Journal Supplement Series, Volume 143, Issue 1, pp. ... Bibliographic Code:* 2002ApJS.. ... 1M We describe a program to identify optical counterparts to radio sources from the VLA FIRST survey using the Cambridge APM scans of the POSS-I plates. We use radio observations covering 4150 deg^2 of the north Galactic cap to a 20 cm flux density threshold of 1.0 mJy; the 382,892 sources detected all have positional uncertainties of ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/FIRST-APM3.html -- 3.6 Кб -- 18.03.2015
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38. STScI NICMOS Software
Next: NICMOS Science Up: NICMOS Data Calibration and Previous: NICMOS Software at the . ... Reference File Tools . Image Analysis and Reduction . ... These include the tasks used in the STScI pipeline, tools to generate the reference files used by the calibration pipeline tasks, and general image analysis, manipulation, and arithmetic tasks. ... Calnica is used to apply instrumental calibrations to individual datasets, while calnicb is used to process associated sets of NICMOS images. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node17.html -- 9.7 Кб -- 12.06.2006
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39. :: Generated By JQueryForm.Com
First Name . Last Name . ... A contributed talk . A poster . ... Tentative title of your oral contribution/poster . Required if ask for a Poster or Talk . ... Required if you are member of a collaboration . Short abstract of your oral contribution/poster . Required if you ask for a Poster or Talk . Options . ... Please select additional options . ... Please check the required fields. Powered by jqueryform.com . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/multispin16/form.html -- 12.0 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/multispin16/form.html -- 12.0 Кб -- 09.04.2016
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40. http://sn.sai.msu.ru/~sil/preprints/postbr2.pdf
... All the galaxies are divided into 4 groups depending on the environment type; every subsample contains more than 10 galaxies. ... An effect of environments is seen both for the nuclei and for the bulges: if we consider the clusters (Virgo and Ursa Ma jor) and group centers as dense environments and the field and group periphery as sparse environments, then in the dense environments the stellar populations of S0s are in average older by 4­5 Gyr than in the sparse ones. ...
[ Текст ]  Ссылки http://sn.sai.msu.ru/~sil/preprints/postbr2.pdf -- 85.0 Кб -- 01.12.2004
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