1. Horsehead and Orion Nebulas
... Credit Copyright: Maurice Toet , Steve Loughran , Darren Jehan Tim Jardine Explanation: The dark Horsehead Nebula and the glowing Orion Nebula are contrasting cosmic vistas. ... Alnitak is the easternmost star in Orion's belt and is seen as the brightest star to the left of the Horsehead . ... Publications with keywords: Horsehead Nebula - Orion Nebula - interstellar medium . Publications with words: Horsehead Nebula - Orion Nebula - interstellar medium . ... Orion: Head to Toe . ...
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http://www.astronet.ru/db/xware/msg/1247401 -- 15.5 -- 05.10.2010
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2. APOD: 2013 October 29 - Horsehead and Orion Nebulas
... 2013 October 29 . Horsehead and Orion Nebulas . ... Explanation: The dark Horsehead Nebula and the glowing Orion Nebula are contrasting cosmic vistas. ... The familiar Horsehead nebula appears as a dark cloud, a small silhouette notched against the long red glow at the lower left. Alnitak is the easternmost star in Orion's belt and is seen as the brightest star to the left of the Horsehead . ... The magnificent emission region, the Orion Nebula (aka M42), lies at the upper right. ...
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http://www.sai.msu.su/apod/ap131029.html -- 5.2 -- 28.02.2014
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3. A collection of images
... The TRACE images may be used without restrictions in publications of any kind. ... These two images, taken on 18 November 2000 at 15:54UT and 16:11UT, respectively, show such an event: the red circle in the image to the left shows a region where many loops are cooling, with bright loop tops (the intensity scales with the square root of the image to reduce the dynamic range). ... See also a collection of images related to the Sun, other cool stars, and solar-terrestrial effects . ... Images | ...
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http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/sun/T171_20001101_101547.html -- 13.0 -- 28.12.2000
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4. Dusty HII Regions and Planetary Nebulae
There is often dust associated with ionized regions. Compact HII regions usually have associated dust from a molecular cloud in which the massive star is being "born". ... For such stars the dust is not produced by the star, and a variety of dust features are observed. The planetary nebulae also usually have associated dust from the previous stage of evolution where they were either carbon stars or M-type giants. ... The feature near 11.5 microns in the IC 418 spectrum may be due to SiC dust. ...
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http://www.stsci.edu/~volk/features3.html -- 6.2 -- 27.05.2014
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5. GSAOI Orion Nebula Cluster Science Page
... GSAOI Home . ... Science . ... Deep imaging at J , H , and K is required to identify all stellar objects, brown dwarfs, and planetary mass objects in the central region of the Orion Nebula Cluster down to masses comparable to that of Jupiter. This is required to establish the initial mass function, i.e., the number of stars of each mass that have formed, in this region of intense massive star formation. ... The fields of the GSAOI detectors are shown as four green squares in each frame. ...
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http://www.mso.anu.edu.au/gsaoi/science/orion.shtml -- 6.7 -- 01.10.2012
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6. Fabry-Perot Interferometer: Gallery Old
... Here some data observed on the 6m telescope with IFP installed in the OLD focal reducer are presented. ... Mkn 3: velocity field . ... NGC 5252: [OIII] image . ... NGC 5252 was observed 23 Feb. 1998 in the [OIII]5007 emission line with CCD TK1024 as detector. ... We observed the ionized gas velocity fields of the spiral galaxies with two purpose. ... Restored velocity field of NGC 157 in the reference frame rotating with the pattern speed overlaid on the Ha image of the galaxy . ... NGC 4100 . ...
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http://mavr.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifp.html -- 9.9 -- 28.12.2007
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http://www.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifp.html -- 9.9 -- 11.09.2010
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http://jet.sao.ru/hq/lsfvo/devices/scorpio/galleries/gal_ifp.html -- 9.9 -- 02.10.2012
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7. M78 off Orion: Bladerunner Nebula? | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... Colin Johnston . ... This submillimetre-wavelength image of the region surrounding the reflection nebula M78 made with the Atacama Pathfinder Experiment (APEX) telescope (overlaid on a view of the same region in visible light) shows the position of interstellar dust grains (orange) to show where new stars are being formed.( ... Here you will find the latest news and views from the fascinating worlds of astronomy and space exploration. ...
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http://www.armaghplanet.com/blog/image-of-the-month-on-fire-off-orion.html -- 41.1 -- 09.04.2016
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8. The giant HII region NGC 3603
... Australia Telescope Compact Array Radio Imaging of the Proplyd-like Objects in the Giant HII Region NGC 3603'' . M?cke, A., Koribalski, B.S. , Moffat, A.F.J., Corcoran, M.F., Stevens, I.R. 2002, ApJ 571, 366 . ... Brenneman, L., Corcoran, M.F., Moffat, A.F.J., Marchenko, S.V., Ptak, A., Skalkowski, G., Mushotzky, R., Stevens, I.R., Mueke, A., Koribalski, B.S. , et al. ... Physical Properties of visual counterparts to X-ray sources in the giant HII region NGC 3603'' . ...
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http://www.atnf.csiro.au/people/Baerbel.Koribalski/ngc3603/ -- 13.4 -- 10.04.2016
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9. Sunspots and active regions October 09, 2014
... Sun images . ... Active areas . October : 2014 . ... The following regions with sunspots can be now observed on the Sun's surface . Group number . ... Group length (in degrees) . ... Alpha . ... Coordinates and other characteristics of active regions are issued for October 09, 2014 00:31 UT The following H-alpha plages without spots can be currently observed on the Sun's surface . ... Coordinates and other characteristics of active regions are issued for October 09, 2014 00:31 UT . ...
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http://www.tesis.lebedev.ru/en/active_areas.html?m=10&d=9&y=2014 -- 26.7 -- 11.04.2016
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10. IDL programs
... This program was created for correlating chosen regions in the series of fts images. ... Chosen regions' . ... In this section the program counts the integral for each region of the grid for each image. ... As a matter of fact, the integral is total brightness of the region and it is counted by 'int_tabulated' IDL function. ... In addition, the program will show the count of the regions which correlate with the corresponding region (the brighter region means the bigger count) and its contour. ...
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http://lnfm1.sai.msu.ru/~kupry/SOFTWARE/korel_en.html -- 9.9 -- 15.08.2003
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11. The Tarantula Nebula
... The Tarantula Nebula , also known as 30 Doradus and NGC 2070 , is a large region of ionized gas surrounding a collection of newly-forming stars at the eastern end of the stellar bar in the Large Magellanic Cloud (many similar regions are scattered through the LMC; see Kennicutt et al. ... The false-color image above is a log-scale display of a mosaic of several images taken with a CCD camera on the 0.6m Curtis Schmidt telescope at Cerro Tololo Inter-American Observatory in December 1994. ...
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http://www.naic.edu/~gibson/30dor/ -- 4.1 -- 19.08.2004
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12. Phil Plait's Bad Astronomy: Bitesize Astronomy
... Bad Astronomy . ... Bitesize Astronomy . ... Last week's Snack talked about how black holes can affect the environment around them in such a way as to be very bright . ... It's a common misconception that black holes always have matter swirling into them. ... As this matter gets closer and closer to the black hole it piles up and a large, fairly flat disk forms. This is called the accretion disk , because matter from this disk accretes (that is, falls in) on the black hole. ... 2008 Phil Plait. ...
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http://www.badastronomy.com/bitesize/jetplane.html -- 21.9 -- 09.04.2016
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13. "Structure" publications in 2005 year
Our publications in 2005 year S.A. Pustilnik (SAO), A.Y. Kniazev (ESO, SAO), A.G. Pramskij (SAO) . Astronomy and Astrophysics, Volume 443, Issue 1, November III 2005, pp.91-102 (11/2005) . ... Kniazev, Alexei Y.; Grebel, Eva K.; Pustilnik, Simon A.; Pramskij, A.G.; Zucker, D.B. The Astronomical Journal, Volume 130, Issue 4, pp. ... 10/2005) . Pustilnik, S. A. Astron. ... Kniazev, A.Y.; Pustilnik, S.A.; Grebel, E.K.; Lee, H.; Pramskij, A.G. VizieR On-line Data Catalog: J/ApJS/153/429. ...
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http://www.sao.ru/precise/Laboratory/Publications/2005_pub.html -- 3.9 -- 25.11.2005
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14. Efimova Ekaterina Andreevna
... Samara State Aerospace University Staff Efimova Ekaterina Andreevna . ... May 2015 - Co-organiser of Regional Student Contest 'Management' (Samara, Samara State Aerospace University); . ... December 2014 - Chair Organizing Committee, Inter-regional Student Contest "Change Management and Organizational Development in the Business" (Samara, Samara State Aerospace University); . April 2014 - Co-organiser of University Student Contest 'Management' (Samara, Samara State Aerospace University); . ...
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http://www.ssau.ru/engstaff/335714904-Efimova-Ekaterina-Andreevna/ -- 27.6 -- 10.04.2016
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15. CMEs and Space Weather
Properties of the Solar Eruptive Event of 19 October 2001, 09:40 UT . ... 1) IZMIRAN, Troitsk, Moscow Region, 142190 . ... Basing on IZMIRAN and NIRFI radio observations, we analyze an event which is characterized by sufficiently intense emission in the cm- and dm-ranges under almost total lack of metric bursts. This peculiarity appears to be caused by very slow speed (V~240 km/s) of a coronal mass ejection (CME) recorded in this event with SOHO/LASCO. ... Coronal Mass Ejections . ...
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http://www.izmiran.rssi.ru/~ichertok/011019/index.html -- 3.6 -- 07.06.2012
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16. Magnetospheric Emission From Isolated Pulsars
Most current theories for magnetospheric emission can be grouped into polar cap, outer gap, and nebular models. These models, at least in some cases, need not be mutually exclusive; the Crab pulsar (among others), for example, shows clear evidence for pulsed emission from the magnetosphere and unpulsed emission from the surrounding nebula. ... This suggestion is strengthened by observation of a distinct soft emission component, consistent with the cooling scenario, from several of these pulsars. ...
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http://hea-www.harvard.edu/~slane/psr/PSR_magnet.html -- 8.0 -- 01.10.2012
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17. AdelePlunkettAstro
... PhD Yale University, Astronomy, 2015 . ... MS, MPhil Yale University, Astronomy, 2011 . ... Plunkett, Adele L. ; Arce, Hctor G.; Corder, Stuartt A.; Dunham, Michael M.; Mardones, Diego; Garay, Guido 2014, ApJ, 803, 22, Assessing molecular outflows and turbulence in the protostellar cluster Serpens South . ... Department of Astronomy Seminar, Universidad de Chile, Santiago, Chile April 2013 . ... Yale-University of Chile Meeting, New Haven, CT December 2011 . ...
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http://www.eso.org/~aplunket/cv.html -- 10.7 -- 15.01.2016
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18. An anarchic region of star formation captured | Astronomy.com
... Tonight's Sky . ... Star Atlas . ... stars . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... An anarchic region of star formation captured . ... RELATED TOPICS: STARS . The star formation region NGC 6559. ... The Danish 1.54-meter telescope located at the European Southern Observatory (ESO) La Silla Observatory in Chile has captured a striking image of NGC 6559, an object that showcases the anarchy that reigns when stars form inside an interstellar cloud. ...
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http://www.astronomy.com/news/2013/05/an-anarchic-region-of-star-formation-captured -- 68.8 -- 10.04.2016
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19. Campaign 2, October 1998
Four spacecraft: INTERBALL Tail probe (IB_TAIL), Auroral probe (IB_AUR), POLAR(NASA/ISAS), GEOTAIL (NASA) are considered. Click icons to make large pictures. ... FSP criteria | FSP ASCII file | Four spacecraft . in the FSP situations . ASCII file . ... Magnetic conjugations . ASCII files : . ... The mulisatellites conjugations : . ... The FSP polar diagram . Click hear for more detailed information about each of four orbits. Last modified 19 October 99 . ... IKI RAN | ...
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http://www.iki.rssi.ru/vprokhor/camp2/199810/9810.htm -- 4.1 -- 19.11.1999
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http://www.cosmos.ru/vprokhor/camp2/199810/9810.htm -- 4.1 -- 19.11.1999
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20. Campaign 2, October 2000 (continue)
Four spacecraft: INTERBALL Tail probe (IB_TAIL), CLUSTER II (ESA/NASA), POLAR(NASA/ISAS), GEOTAIL (NASA) are considered. ... four spacecraft . ... INTERBALL . ... IB_TAIL) . ... NASA) . GEOTAIL . NASA, ISAS) . The four spacecraft . ... Modified 28 August 2000 . ... INTERBALL mission | ...
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http://www.iki.rssi.ru/vprokhor/camp2/200010/0010cnt.htm -- 4.3 -- 01.09.2000
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