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1. Stellar Astronomy
... Subject and Problems of Stellar Astronomy. ... Plane of Galaxy, Methods of Its Location Determination. ... Stars Distances. ... Other Methods of Stars Distances Determination. ... Tangential Velocities, Their Determination by Self-Motions. ... Determination of Solar Apex and Spatial Velocity by Radial and Spatial Velocities of Stars. ... Features of Orientation and Parameters of Peculiar Stellar Velocities Ellipsoid. ... General and Selective Light Absorption in Galaxy. ... Darc Clouds in Galaxy. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/zor_astron_e.html -- 8.0 Кб -- 23.02.2005
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2. Conference location directions
Getting to Moscow from the airport: There are three international airports in Moscow: Sheremet'yevo , Domodedovo , and Vnukovo . All three are connected to Moscow through a high-speed railway, called Aeroexpress , with moderately priced tickets (320 rubles, approx. ... The point of arrival is a rail terminal, which is connected to a subway station: Byelorusskaya for Sheremet'yevo, Paveletskaya for Domodedovo, and Kievskaya for Vnukovo. The map of Moscow Metro (subway) is found in Wikipedia. ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/lifr/Sossinsky2012/directions.htm -- 5.5 Кб -- 21.09.2012
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3. In what direction and at what speed is the solar system moving through the
... Tonight's Sky . ... Sky this Month . ... solar system . ... milky way . ... The Sky This Week: April 1 - 10 . ... Sky this Week . ... Observe the Solar System . Astronomy for Kids . ... Tour the Solar System . ... In what direction and at what speed is the solar system moving through the Milky Way? ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ... Join Astronomy for America's 2017 total solar eclipse! ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/magazine/ask-astro/2008/11/in-what-direction-and-at-what-speed-is-the-solar-system-moving-through-the-milky-way -- 63.1 Кб -- 10.04.2016
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4. Parallax
... The greater the distance, the smaller the parallax. ... That triangle has the same proportions as the much larger triangle ABC, and therefore, if the distance B'C to the thumb is 10 times the distance A'B' between the eyes, the distance AC to the far landmark is also 10 times the distance AB. ... The most distant objects our eyes can see are the stars, and they are very far indeed: light which moves at 300,000 kilometers (186,000 miles) per second, would take years, often many years, to reach them. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/STARGAZE/Sparalax.htm -- 7.1 Кб -- 21.12.2007
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5. Infall and Omega
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[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/1997/ph410/l12.html -- 4.5 Кб -- 07.02.1997
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6. Astronomy Outreach Images Workshop (ORIWORKS)
Workshop Home . ... Travel to Baltimore . ... Baltimore, MD 21218 USA . ... Travel options between Washington, D.C. and Baltimore are discussed below for those participants that will also be attending the "Communicating Astronomy to the Public Conference that immediately follows this workshop on October 1-3, 2003 in Washington D.C. ( http://www.nrao.edu/ccap/ ). ... Airport: The closest is Baltimore-Washington International Airport (BWI), which is about 13 miles (25 minutes) from the Institute. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/oriworks_dev/stsci.html -- 13.1 Кб -- 26.09.2003
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7. Siding Spring Survey
T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~rmn/ -- 11.4 Кб -- 23.12.2011
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8. Location of slitlets and flat-field correction
... The very first step after correcting bias, dark, and overscan is to find the edges of the slitlets. This is done by the command LOCATE/MOS . This command takes the central trace of a flat-field and detects the edges of the slitlet by simple threshold comparison. ... The offsets in dispersion direction between the slitlets will be read from the header of the flat-field frame for FORS data and stored in :xoffset . ... The actual flat-correction is then performed with COMPUTE/IMAGE . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node679.html -- 4.0 Кб -- 23.02.1996
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9. News Results
This source is hiding behind our Galaxy at a distance of ~18 Mpc, located at a galactic latitide of 0 degrees. ... As we look towards longer wavelengths, 60 micron, to try and penetrate the Galactic Plane, we still see confusion from galactic sources. ... If the image seems some what confusing that is because the MOST is a continuum radio telescope and when it looks in the direction of our Galaxy it detects radiation from sources within our Galaxy and from sources that may lie behind our Galaxy. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/multibeam/results.html -- 5.9 Кб -- 01.10.2012
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10. Frontiers of Astronomy with the World's Largest Radio Telescope Frontiers of
Hall of the States Building . 444 North Capitol St., NW . ... The Hall of the States Building is directly across the plaza from Union Station. ... Head right on Massachusetts Avenue for less than one block and take a left onto North Capitol Street (heading towards the U.S. Capitol). The building is on your right at 444 North Capitol Street. Important Note: The Hall of the States Building has security, and therefore checks visitors against the list of participants. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~astro/frontiers/location.shtml -- 3.4 Кб -- 02.10.2012
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11. Spatial distribution of X-ray binaries at the Galactic center after the
... As is known, the observed distribution of massive stars in the direction of the Galactic center looks very peculiar: the vast majority of all massive stars are concentrated towards the central 1 pc or so (Genzel et al. ... In order to compare the observed distribution of X-ray sources in the Galactic center with what would be expected from the population synthesis computations, we have considered two hypothetical scenarios for the location of the starburst. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~polar/html/publications/apj/node9.html -- 12.0 Кб -- 21.06.1996
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12. Vortex structure of NGC 157.
Restored velocity field of NGC 157 in the reference frame rotating with the pattern speed overlaid on the H_alpha image of the galaxy. ... The line-of-sight velocity fields of gaseous clouds in galactic disks of NGC 157 were analyzed by the method of reconstruction of 3D vector velocity field --- three components of velocities. ... This figure is produced with the help of software VORTEX developed in the Institute of Astronomy of the Russian Academy of Sciences. ... Back to Project Vortex. ...