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41. Journal "Peremennye Zvezdy"
M55 Color Magnitude Diagram . ... B.J. Mochejska , J. Kaluzny ( CAMK ), 1m Swope Telescope Explanation: This color "picture" of globular star cluster M55 may not look like any star cluster you've ever seen. ... In the picture, a Color Magnitude Diagram (CMD), M55's individual stars are represented as dots whose color indicates relative temperature, red (cool) to blue (hot). ... The broad swath extending diagonally from the lower right is the cluster's main sequence . ... Specific rights apply . ...
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Ссылки http://www.astronet.ru/db/varstars/msg/1166377 -- 8.6 Кб -- 23.02.2001
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42. (Type a title for your page here)
style html {overflow-x:hidden; } html, body { height: 100 %; margin: 0px ;padding: 0px ; }#__container { position :relative; min-height: 100 %; }#__footer{ position :absolute; bottom:65px; width: 100 %;}#__ mlk { width: 100 % ! important ;border-top:1px solid #AEAEAE;border-botton:1px solid #AEAEAE;z-index:999 ! important ; color : black ! important ; position : absolute! important ;left: 0px ! ...
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Ссылки http://www.epizodsspace.narod.ru/kosm/t/tonini_mishel/tonini_mishel.html -- 3.9 Кб -- 09.04.2016
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43. General Astrometry
General Knowleges about Astrometry. ... Universal Tool, Meridian Tool, Meridian Circle, Vertical, Photografic Zenithal Telescope, Astrolabe, Zenith Telescope, Horizontal Meridian Circle, etc. Meridian Principle of Objects' Coordinates Determination. ... Absolute and Relative Methods of Coordinates Determination. ... Photografic Method in Astrometry. Telescopes for Position Observations by Photografic Method. ... Basis and Theory of Photografic Method of Coordinates Determination. ...
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Ссылки http://space.univ.kiev.ua/courses/zag_astromet_e.html -- 4.1 Кб -- 23.02.2005
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44. TIME DILATION - an Astronomy Net Observation_reports Forum Message
Astronomy Discussion Forums . Forums: . ... TIME DILATION . ... Time dilation is what we take to be the disagreement in the total time of an event as measured by a moving frame and stationary frame. ... Imagine a car 100km from a stationary observer and which is positioned such that it would travel 200km on a straight line in a direction away from the stationary observer. ... Therefore the total time of motion of the car as measured by the stationary observer is T= t- 100km/C + (100km+200km/C). ...
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Ссылки http://www.astronomy.net/forums/observation_reports/messages/302.shtml -- 20.3 Кб -- 09.04.2016
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45. Amateur Astronomers Association of New York ? Amateur Astronomers Association
... Observing . ... Solar Observing . ... April 3 (SUN) - Solar Observing, Central Park , Manhattan . ... APRIL'S SKY . ... Lecture Series at the American Museum of Natural History The Amateur Astronomers Association is proud to present an astronomy lecture series from October through May each year for our members and the .. ... The€аAmateur Astronomers Association of New York€аwas organized in 1927 to promote the study of Astronomy, emphasizing its cultural and inspirational value. ...
46. Restrictions on the Scenario Parameters
... we show that the comparison between the calculated and observed numbers of the most ``fragile'' (from the point of view of the binary evolution scenario ) galactic binary types (such as X-ray low-mass X-ray binaries (LMXB), cataclysmic variables (CV), Be-stars with compact companions, relative number of visible binary radiopulsars with normal and compact secondary components) impose certain constraints on the feasible initial ... Phenomenological Kick Velocity . ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node41.html -- 6.6 Кб -- 26.02.1997
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47. http://www.issp.ac.ru/iao/2015/booklet/b11_ia15_p_en_b.pdf
... The extinction in terrestrial atmosphere. ... 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. ... Calculate the air mass for given zenith distances in 1st 54.9 11800 column, and write the result into the 2nd column. ... Spectral observations. ... Calculate the radial velocity Vr of the star on each date, the results of measurements and write calculations into the table. ...
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Ссылки http://www.issp.ac.ru/iao/2015/booklet/b11_ia15_p_en_b.pdf -- 169.3 Кб -- 03.12.2015
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48. http://www.izmiran.rssi.ru/services/saf/archive/en/2014/obzor20141018.en.txt
Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 13 - 17.10.2014, Forecast on 18 - 27.10.2014, Carrington Rotations 2155, 2156 (17,72.09; 15,00.10.2014) SUNSPOT-FORMING ACTIVITY OF THE SUN WAS AT THE AVERAGE LEVEL. ... NEXT WEEK THE AVERAGE AND LOW LEVELS OF SUNSPOT-FORMING ACTIVITY IS EXPECTED. ... BY DATA OF CORONOGRAPHS SOHO AND STEREO WERE OBSERVED 20 CME, ONE OF WHICH WAS THE "HALO" TYPE AND TWO - "PARTIAL GALO II". ... TODAY ENERGY OF LAST MAGNETIC FLUX IS SPENT. ...
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Ссылки http://www.izmiran.rssi.ru/services/saf/archive/en/2014/obzor20141018.en.txt -- 6.1 Кб -- 18.10.2014
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49. source comment
... The derived position here agrees with the position from recent ATCA observations, RA=15h 01m 34.74s, Dec=39 18 39.2" (Tasker, private communication) which found the source unresolved. Because of the relatively large position offset, the reality of the fainter component 0.12" to the west is somewhat in doubt. However, the ATCA centroid position is offset by 0.3" to the south-east of the VLBA position, suggesting that the faint component may be part of more extended structure. ...
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Ссылки http://www.vsop.isas.ac.jp/VLBApls/J1501-3918.comment.htm -- 1.8 Кб -- 16.10.2000
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50. http://hea.iki.rssi.ru/integral06/papers/D32_Khamitov01-04Oct06_10:26:31.pdf
... R-band images obtained at 0.8 arcsec seeing conditions have allowed us to separate foreground star from point-like extragalactic source and estimate their brightness separately. ... To study the nature and properties of the source, we observed it under high spatial resolution. ... CONCLUSION RTT150 optical observations with sub-arcsecond seeing and low resolution spectra confirm the hypothesis of superposition of a radio source onto a `normal' F/G galactic star proposed by [1]. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/D32_Khamitov01-04Oct06_10:26:31.pdf -- 635.3 Кб -- 04.10.2006
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51. http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf
Microsymposium 38, MS083, 2003 (A4 format) MERCURY: LOCAL VARIATIONS OF THE PHOTOMETRIC RELIEF. ... Because of trajectory and pointing angle constraints the planet could be observed from Mariner 10 only over a small range of phase angles between about 75o and 110o. Therefore the photometric investigations are restricted to measuring the distribution of brightness on the Mercurian disk. ... Raw versions of real-time processing pictures FDS 0000984 and FDS 0000986 were used (images 196 and 202). ...
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Ссылки http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf -- 346.6 Кб -- 06.10.2008
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52. –А observer : V–їnus, Spica et des –їtoiles filantes | Ciel et Espace
... Ciel Espace, le magazine qui vous guide toujours plus loin . ... des actualit–їs . ... les plus belles images de l'Univers d–їcrypt–їes pour vous . ... Accueil –А observer : V–їnus, Spica et des –їtoiles filantes . ... Surveillez aussi les –їtoiles filantes . Lorsque le ciel devient sombre, il se peut que quelques m–їt–їores z–Rbrent le ciel, car c'est actuellement le pic d'activit–ї de l'essaim d'–їtoiles filantes des Aurigides . ... 08/08/2013 - Les Nuits des –їtoiles 2013 : cвАЩest parti ! ...
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Ссылки http://www.cieletespace.fr/node/5836 -- 29.9 Кб -- 09.04.2016
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53. Captions
... The CAPTION element is used to label a table or figure. Use the align attribute to specify the position of the caption relative to the table/figure. ... CLASS . ... The CLASS attribute is most commonly used to attach a different style to some element, but it is recommended that where practical class names should be picked on the basis of the element's semantics, as this will permit other uses, such as restricting search through documents by matching on element class names. ... ALIGN . ...
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Ссылки http://comet.sai.msu.ru/webdesign/html-3.0/captions.html -- 3.0 Кб -- 19.12.1996
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54. Linear polarization: wavelength dependence
... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...
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Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/ASTNOTES/node7.html -- 18.9 Кб -- 19.11.2010
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55. Relative literature to radio galaxy study
... High redshift radio galaxies . ... Verkhodanov O.V., Kopylov A.I., Zhelenkova O.P., Verkhodanova N.V., Chernenkov V.N., Parijskij Yu.N., Soboleva N.S., Temirova A.V. 2000. ... Verkhodanov O.V., Kopylov A.I., Parijskij Yu.N., Soboleva N.S., Temirova A.V. "Color ages of parent galaxies of high redshift radio sources", in Proc. XV Conf. on "Aktualnye problemy vnegalakticheskoi astronomii" ("Current Problems of Extragalactic Astronomy"), Pushchino, May 25--29, 1998, printed in Pushchino Sci. ...
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56. AAL Homepage
... ARTICLE: The Adventurous Search For The Astronomical Unit . ... Kepler himself had suggested to use the rare occasions of Venus transiting (crossing) the solar disk to measure our distance to the planet. ... Due to the orbital inclination of Venus against the ecliptic of 3.5°, a Venus transit is so rare that it happens only at intervals of 121.5 years, 8 years, 105.5 years, 8 years and so on. ... Crabtree witnessing the transit of Venus 1639 . ... Transits of Venus - The Quest for the Solar Parallax...
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Ссылки http://www.aal.lu/SPECIAL_TOPIC/2/ -- 29.5 Кб -- 09.04.2016
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57. Elena Seifina
... Field of interest: data analysis and interpretation of X-ray observations of BHC and NS systems, astrophysics of compact objects and related phenomena: X-ray , optical and radio observations , shocks and stellar winds, emission mechanism, the spectral and timing analysis of the X-ray emission from microquasars ( signature of accreting BH), atoll- and Z-sources ( signature of accreting NS), modeling of INTEGRAL images % . ...
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Ссылки http://uranus.sai.msu.ru/~seif/ -- 2.2 Кб -- 11.04.2013
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58. Observing for Students and Visitors
... Moore Observatory is a research and advanced teaching facility of the University of Louisville. ... The 24-inch Ritchie Chretien (RC24) telescope is a research instrument used by faculty and graduate students involved in studies of exoplanets, optical properties of the atmosphere, and the development of imaging and spectroscopic technology. ... Kent (CDK20S) are collaboratively operated by the University of Louisville and the University of Southern Queensland for both research and education. ...
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Ссылки http://www.astro.louisville.edu/moore/visit/index.html -- 3.6 Кб -- 18.10.2010
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59. observing | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... Armagh Planetarium . ... Space Flight . ... Posted on April 6, 2016 | No Comments Spring has truly sprung. ... Continue Reading.. Posted on March 1, 2016 | ... Posted on February 2, 2016 | No Comments Goodbye January blues, hello February fun! ... Posted on January 7, 2016 | ... Posted on November 4, 2015 | ... Posted on October 5, 2015 | ... Posted on September 3, 2015 | ... Posted on August 3, 2015 | ... Posted on June 25, 2015 | ...
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Ссылки http://www.armaghplanet.com/blog/tag/observing -- 58.2 Кб -- 09.04.2016
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60. SSAU improved its position in two Russian ranking at once
... Pre-university education . ... For the year Samara State Aerospace University moved up in the ranking of Vladimir Potanin Foundation from the 44th to the 10th place and added three positions in the ranking of universities reputation Expert RA in the field of Engineering, natural and exact sciences . Samara State Aerospace University has significantly improved its position in the ranking of universities of Vladimir Potanin Charitable Foundation at the end of academic year 2014-2015. ...
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Ссылки http://www.ssau.ru/engnews/11771/ -- 25.4 Кб -- 11.09.2015
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