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1. A Close Encounter Of The Stellar Kind
Astronomy Picture of the Day . A Close Encounter Of The Stellar Kind . ... Explanation: The unassuming star centered in this sky view will one day be our next door stellar neighbor. ... Known in catalogs of nearby stars as Gliese (Gl) 710 it is predicted to come within nearly 1 light-year of the Sun ... about 1.5 million years from now. ... NASA Official: Jay Norris. ... Publications with keywords: Gliese 710 - nearby - star . Publications with words: Gliese 710 - nearby - star . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1169750 -- 15.1 Кб -- 10.07.2001
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2. APOD: June 26, 1997 - A Close Encounter of the Stellar Kind
... June 26, 1997 . A Close Encounter of the Stellar Kind . Credit: Digitized Sky Survey , SkyView . Explanation: The unassuming star centered in this sky view will one day be our next door stellar neighbor . ... This future stellar encounter was discovered by researchers Joan Garcia-Sanchez and Robert Preston ( JPL ), and collaborators while studying stars in the solar neighborhood using data from the Hipparcos Astrometry Satellite . ... About APOD > . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap970626.html -- 5.1 Кб -- 02.10.2012
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3. A gallery of interacting galaxies
... Home . OOF . ALMA . ... Interacting galaxies . ... OOF Index . ... Low redshift close pairs . This pages illustrates some of the galaxies with close pairs which we identified in our study of star formation in interacting galaxies selected from the Sloan Digital Sky Survey (Nikolic et al 2004, see the publication list ). ... The pixel scale in approximately 0.4 arcseconds and colour is approximately true-colour. Images and data courtesy of the Sloan Digital Sky Survey . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/galevol/interactgallery.html -- 10.2 Кб -- 25.11.2009
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4. The Database of Close Binary Systems
The Database of Close Binary Systems . ... Team . ... This web-based interactive database is being developed and maintained by a team at the Sternberg Astronomical Institute of the Moscow State University . The project is an on-line extension of our catalogue on "Highly Evolved Close Binary Stars" (volumes I, II) published by Gordon and Breach in 1996. As of November 2009, the database (both the software and the content) is in its development/testing phase. Sternberg Astronomical Institute ...
[ Сохраненная копия ]  Ссылки http://uranus.sai.msu.ru/cbs/ -- 7.0 Кб -- 01.10.2012
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5. Kepler 36b and c: Too Close for Comfort | Astronotes
... Planets . ... Earth Satellites . ... Looking in the direction of the constellation Cygnus the Swan and launched by NASA in 2009 is the Kepler Space Observatory.Many previous missions searching for exoplanets mainly detected large giant planets, like large hot Jupiters (it is easier to detect larger planets).However KeplerтАЩs main objective is to search for much smaller planets located in a habitable zone which is not too close nor too far from their star; planets which may be just like our Earth. ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/too-close-for-comfort.html -- 46.3 Кб -- 09.04.2016
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6. http://www.wro.org/scodova/RNGC_by_Abell347.pdf
... 12, 2015 Abell 347 MAC 0223+4140 Sep 14 2012 36 And And And And Galaxy Galaxy Galaxy Galaxy 17mmT4 EF,ES,STELLAR OR VERY CLOSE TO F*,SUSP, AGC 347 ,R=P MAC 0223+4159B Sep 14 2012 36 17mmT4 EF,VS,ELONG,UB,CLOSE TO *, AGC 347 ,R=P MAC 0224+4130 Sep 14 2012 36 17mmT4 EF,VS, PATCH ,AV COMES AND GOES, AGC 347 ,R=P MAC 0224+4136 ...
[ Текст ]  Ссылки http://www.wro.org/scodova/RNGC_by_Abell347.pdf -- 11.4 Кб -- 13.04.2015
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7. About laboratory
Laboratory of Stellar Physics . ... A study of close binaries with black holes, neutron stars and white dwarfs. ... A study of SS433 - the massive close binary with a black hole in the regime of supercritical accretion . ... A search for intermediate-mass black holes (IMBH). The black holes which are not supermassive black holes observed in quasars, and which were formed not in massive stars. ... A search for new magnetic stars, new CP stars, measurements of magnetic fields in stars . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/jet/eng_about.html -- 6.9 Кб -- 11.11.2015
[ Сохраненная копия ]  Ссылки http://www.sao.ru/jet/eng_about.html -- 6.9 Кб -- 11.11.2015
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/eng_about.html -- 6.9 Кб -- 11.11.2015
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8. The Database of Close Binary Systems
The Database of Close Binary Systems . ... Team . ... This web-based interactive database is being developed and maintained by a team at the Sternberg Astronomical Institute of the Moscow State University . The project is an on-line extension of our catalogue on "Highly Evolved Close Binary Stars" (volumes I, II) published by Gordon and Breach in 1996. As of September 2009, the database (both the software and the content) is in its development/testing phase. ...
[ Сохраненная копия ]  Ссылки http://dionis.sai.msu.ru/cbs/ -- 6.5 Кб -- 01.10.2012
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9. First Observation of a Close Earth-Approaching Near-Earth Asteroid Using the
... Figure 8: Can you detect the motion of the near-Earth asteroid 2000PH against the background stars during its close approach to Earth around 27 July 2004? ... Down) observed and imaged the unusual near-Earth asteroid 2000PH during its close approach to the Earth around 27 July 2004. The observations were carried out remotely using the new 2m aperture Faulkes telescope situated on the 10,000-foot summit of Haleakala, on the island of Maui in Hawaii. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep2004/node65.html -- 7.5 Кб -- 19.04.2005
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10. Los Cielos de Am , The darkest sky and the two galactic hemispheres
I was wondering what conditions should be met to have the "darkest" sky .. ... Upon the above publication of the Southern Galactic hemisphere, TunГ Tezel started seeking opportunities to create the Northern counterpart image. ... So, the initial quest of having the darkest possible sky have delivered us these two all-sky images of the two galactic hemispheres as seen from Planet Earth. Zoomable and 'full-screenable' fisheye view of the "darkest sky" Southern Galactic Hemisphere image. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~sguisard/Pagim/darkest_sky.html -- 22.9 Кб -- 18.05.2011
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11. Closer view
. Search this album . Gallery . :: The 2003 fires . :: Photos of the 74" after the fire, by KimтАж . :: Closer view . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . View full size . Title: Closer view . File name: KR74k.jpg . Dimensions: 540 x 360 px . Page: 1 2 3 4 5 6 7 8 9 10 12 13 . Powered by Gallery 3.0.9 (Chartres) . Login
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gallery3/index.php/fires2003/Kim-Rawlings/KR74k -- 14.1 Кб -- 10.04.2016
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12. The Grus-Quartet
B?rbel Koribalski ( ATNF ) . ... The Grus-Quartet consists of four large spiral galaxies which are so close to each other that they should be interacting. The high starburst activity of two of the members, namely NGC 7552 and NGC 7582, is also thought to arise from tidal galaxy-galaxy interactions and subsequent formation of a bar in the disk. ... The colour gradient is in units of Jansky/beam km/s.) . The colour gradient is in units of km/s.) . ... Baerbel.Koribalski @ csiro.au ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Baerbel.Koribalski/ngc7582/grus_hi.html -- 4.4 Кб -- 23.12.2007
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13. cband stability with shutter closed
The stability of the cband receiver/ iflo was measured on 09feb11 during the day. cband receiver centered at 4745. shutter on cband receiver closed (receiver looks at absorber load). 7 iflo bands selected at: 4325,4466,4608,4750,4892,5034, and 5176 . ... The total power was computed for each sample,pol, and band by averaging the 8192 channels of each spectra. ... The vertical lines mark every 600 seconds (to help align things in adjacent bands). total total power varies 0 to 2% of tsys . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/calcb/stability_shutterclose_09feb11.html -- 5.0 Кб -- 04.04.2011
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14. How close can stars get to each other in galaxy cores? | Astronomy.com
... Tonight's Sky . ... Observing . ... Star Atlas . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Astronomy for Kids . ... Get to Know the Night Sky . ... How close can stars get to each other in galaxy cores? ... Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/magazine/ask-astro/2006/01/how-close-can-stars-get-to-each-other-in-galaxy-cores -- 62.9 Кб -- 10.04.2016
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15. Space Projects Closed
... Projects . ... Space Projects . ... Closed . ... Complex Orbital Magneto-plasma Autonomous Small Satellite . ... 1991-1999) . ... Complex Orbital Near-Earth Solar Observations (1994-2001) . ... Active Plasma Experiments (1991-1999) . INTERCOSMOS 19 : launched February 27, 1979 . ... Интеркосмос-25 (АПЭКС) (1991-1999) . ... Интеркосмос-19 (1979-1982) . Интеркосмос-18 (1979) . Цикада (1979) . ... Марс-3 (17.05.1971) . ... Электрон-4 (1964-1965) . ... Космос-49 (1964) . ... 1962) . ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/projects/space/closed -- 11.6 Кб -- 09.04.2016
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16. Maison Close - Jardin Imperial - Пояс для чулок - Черный-золотой цвет
... title='Maison Close - Jardin Imperial - Пояс для чулок - Черный-золотой цвет' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> . Цвет Пурпурный . ... Цвет: слоновая кость, . ... Цвет: черный . ... Цвет: голубой . ... Idigo Масса для моделирования 12 цветов 240 г - Idigo - Idigo . ...
[ Сохраненная копия ]  Ссылки http://astrokuban.info/astroku6809.html -- 22.4 Кб -- 14.02.2016
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17. The First Infrared Study of the Close Environment of a Long Gamma-Ray Burst
We present a characterization of the close environment of GRB 980425 based on 5-160 ЮМm spectro-imaging obtained with Spitzer. The gamma-ray burst GRB 980425 occurred in a nearby (z = 0.0085) SBc-type dwarf galaxy at a projected distance of 900 pc from an H II region with strong signatures of Wolf-Rayet (WR) stars. ... This atypical property is rarely observed among morphologically relaxed dwarfs, suggesting a strong causal link with the gamma-ray burst (GRB) event. ... ADS Citation Query . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2012ApJ...746....7L.html -- 5.0 Кб -- 21.01.2016
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18. Closing down
... First of all, you can obtain a map of the final coordinates of your objects and guide stars by using the command: PLOT/OPTOPUS [table] [label] [EW_flag] , . where [table] is the table output by REFRACTION/OPTOPUS . ... In order to avoid object misidentifications at a later stage, and for a cross identification between object identifiers and hole numbers, it is recommended to bring a printout of the table output created by the command REFRACTION/OPTOPUS to the telescope. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node544.html -- 6.3 Кб -- 23.02.1996
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19. ASP: Editorial: Climbing a Little Closer
home publications > mercury . SEARCH ASP SITE: Match ALL words Match ANY word . ... Editorial: Climbing a Little Closer . ... In the late 1950s, my uncle Morgan and his best friend, Gerald, were using my uncle's small telescope to look at the night sky. ... Sputnik spurred them like so many others to build ships to climb into the sky, to join that chilly, violent Universe that embraces our little warm droplet of life. ... Yet they climbed higher each successful shot. ... Trying to climb higher. ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/pubs/mercury/0002/edit.html -- 17.6 Кб -- 20.04.2012
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20. CH Cyg
... The hot component shows very spectacular activity: irregular outbursts accompanied by fast, massive outflows and jets. ... Diffraction-limited images for both components of CH Cyg binary system were reconstructed using visible speckle interferometry at BTA 6-m telescope (Fig.1). The orbital period 15.6 years and masses: 2.0 Msun and 0.7 Msun for red giant and white dwarf, respectively were derived from angular distance (0.042") and magnitude difference (2 m ) of the components. ... Fig.1. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2010/CHCyg/ -- 4.2 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/SciNews/2010/CHCyg/ -- 4.2 Кб -- 02.10.2012
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