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81. Practical 1 / 8 Ebony Violin Peg Instrument Accessory Laroom Платье Basic-172
... Practical 1 / 8 Ebony Violin Peg Instrument Accessory . Size: SIZE 1 / 8 . ... Type: Violin Peg . For: Violin . Material: Ebony . ... Product size (L x W x H): 6 x 1.8 x 0.7 cm / 2.36 x 0.71 x 0.28 inches . Package size (L x W x H) : 7 x 3 x 2 cm / 2.75 x 1.18 x 0.79 inches . Musical Instruments . ... Package Contents: 1 x Violin Peg . ... Повседневные (casual) платья . ...
[ Сохраненная копия ]  Ссылки http://astrokuban.info/astroku4876.html -- 23.3 Кб -- 14.02.2016
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82. 2dF QSO Redshift Survey (2QZ)
The 2dF QSO Redshift Survey (2QZ) . ... Before jumping into all the finer details of teh survey, a brief non-astronomer's guide to redshift surveys is available. ... The primary scientific aims of the QSO survey are: (1) to obtain the primordial fluctuation power spectrum out to COBE scales, (2) to determine the rate of QSO clustering evolution in the non-linear and linear regimes and hence obtain new limits on the value of and the bias parameter, (3) to apply a powerful geometric method to measure . ...
[ Сохраненная копия ]  Ссылки http://www.2dfquasar.org/ -- 7.8 Кб -- 17.06.2008
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83. Trajectory report
... The OC "Mir" orbit parametres before the final burns . ... Orbit period (in min) . ... Mean orbit altitude (km) . ... solar F 10.7 flux . ... F 10.7 <= 100 - low level; 100 < F 10.7 < 150 - medium level; F 10.7 >= 150 - high level . Orbit 86328(15) - the first burn bulding the descent orbit  D V 1 =9.3 m/s. After burn altitude H min = 188.2 km, H max = 219.2 km. Orbit 86329(16) - the descent orbit second impulse D V 2 =10.4 m/s. After burn altitude H min = 158.9 km, H max = 218.5 km. ...
[ Сохраненная копия ]  Ссылки http://www.mcc.rsa.ru/www_old/Mir/www_eng/MIR/BNO/spr.htm -- 17.2 Кб -- 28.05.2014
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84. http://www.simfov.ru/history/?type=forprint
[invalid parameters to operator level]
[ Сохраненная копия ]  Ссылки http://www.simfov.ru/history/?type=forprint -- 1.0 Кб -- 01.10.2012
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85. http://www.gpad.ac.ru/collaborations/inasan.pdf
The new view on the population of Galactic open clusters A.E.Piskunov1, N.V.Kharchenko2, S.RЖser3, E.Schilbach3, R.-D.Scholz4 1 2 3 4 Institute of Astronomy, Moscow, Russia Main Astronomical ... Observatory, Kiev, Ukraine Astronomisches Rechen-Institut, Heidelberg, Germany Astrophysikalisches Institut Potsdam, Germany What are open clusters and what do they teach us Groups of Population I ... Cluster complexes: OCC-1 = Gould's Belt cluster complex? ...
[ Текст ]  Ссылки http://www.gpad.ac.ru/collaborations/inasan.pdf -- 2655.7 Кб -- 05.07.2006
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86. The new concept of formation and development of the Solar system
... part 2 | ... Part 1 . The new concept of formation and development of the Solar system. ... Thus, the initial pulse of the rotation of a protosolar cloud of the solar system was determined as a result of the diversion of a part of the moment of the rotational pulse of the Galaxy. ... Besides this new approach to the pre-solar system as a system of the destroyed vortex structure, we can understand now a number of other peculiarities of the Solar system's structure. ...
[ Сохраненная копия ]  Ссылки http://www.lermus.ru/users/trunaev/part1.htm -- 28.0 Кб -- 04.12.2001
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87. THEOS SC Injection Accuracy
... Dnepr Cluster Mission 2013 19 June 2014. ... The SC actual injection accuracy was assessed by comparison of the nominal design orbit, with the account for disturbances at separation, and the actual orbit determined on the basis of: . ... With reference to the above data, one can see that deviations of the THEOS osculation orbit parameters at the time of SC separation during Dnepr launch on October 1, 2008 did not exceed the prediction the THEOS SC was launched with high accuracy. ... Mission profile...
[ Сохраненная копия ]  Ссылки http://www.kosmotras.ru/en/news/48/ -- 10.7 Кб -- 09.04.2016
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88. New technique measures mass of exoplanets | Astronomy.com
... New technique measures mass of exoplanets . ... Now, scientists at the Massachusetts Institute of Technology (MIT) have developed a new technique for determining the mass of exoplanets using only their transmission spectra dips in light as a planet passes in front of its star. ... To determine the mass of an exoplanet using transmission spectroscopy, de Wit relied on the effect that a planet s mass has on its atmosphere, as transmission spectra give information on a planet s atmospheric properties. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/news/2013/12/new-technique-measures-mass-of-exoplanets -- 71.7 Кб -- 10.04.2016
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89. StarCalc Home Page [English]
... About StarCalc . News . ... StarCalc Home Page . Short description of changes, implemented in the StarCalc, . ... CHANGES OF PROGRAM CORE FUNCTIONS. CHANGES OF PROGRAM INTERFACE. CHANGES OF OBJECT INTERFACES. ... New "Output console". ... Information, which is generated by StarCalc, is added into the console - for example, ephemeris tables. ... In the StarCalc state file can be saved autorotation parameters, object selection, object locking mode, auto start and stop autorotation mode. ...
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