We present a mid-infrared analysis of star-formation activity in the Large Magellanic Cloud's molecular ridge (south of 30 Doradus). The Magellanic Clouds are a rare laboratory in which extragalactic star-formation diagnostics can be tested at high spatial resolution. ... Detailed analysis in very nearby galaxies, like the Magellanic Clouds, allows us to test and better understand the scaling relations used in unresolved and distant star-formation regions. ...

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... Science User Portal . ... ESO, the European Southern Observatory . ... Travel and Contacts . Travel to ESO Headquarters . ... Survey Telescopes . ... Star Clusters . ... Stars@ESO . ... ESO Science Newsletter . ... As we close in on part of the small constellation of Corona Australis we start to see faint clouds and in the final part of the video the full glory of the dramatic star formation region NGC 6729 is revealed in a new image from the FORS1 instrument on ESOтАЩs Very Large Telescope. ...

... Infrared Portrait of the Large Magellanic Cloud . ... Credit Copyright: ESA / NASA / JPL-Caltech / STScI Explanation: Cosmic dust clouds ripple across this infrared portrait of our Milky Way's satellite galaxy , the Large Magellanic Cloud. ... The dust temperatures tend to trace star forming activity. ... Dominated by dust emission, the Large Magellanic Cloud's infrared appearance is different from views in optical images . ... Close Comet and Large Magellanic Cloud . ... The Large Cloud of Magellan...

Astronotes Armagh Planetarium's Stellar Blog! ... Armagh Planetarium . ... Stars . ... Space Flight . ... Although they look tranquil here, observed up close such young stars would seethe and glare violently. ... Once thought to be a satellite of our own galaxy, increasingly the Small Magellanic Cloud is believed to be an interloper from the intergalactic void which has wandered into its present location and will eventually recede away into the darkness. ... Your email address will not be published. ...

True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR . ... SNR 0453-68.5 . ... DEM L50 . DEM L71 . ... SNR 0509-67.5 . ... SNR 0519-69.0 . ... SNR 0534-69.9 . DEM L238 . ... SNR 0540-69.3 . ... DEM L316A . SNR 0548-70.4 . SNR 0550-68.3 . ... DEM S125 . Chandra Supernova Remnant Catalog . ... Galactic SNR | ...

... 2006 September 4 . The Large Magellanic Cloud in Infrared . ... To help find out, a team of researchers took the most detailed image ever of gas clouds and dust in the neighboring Large Magellanic Cloud (LMC) galaxy. ... Visible are vast clouds of gas and dust , showing in graphic detail that dust prefers regions near young stars (red-tinted bright clouds), scattered unevenly between the stars (green-tinted clouds), and in shells around old stars (small red dots). ... About APOD | ...

... The Large Magellanic Cloud is a Dwarf Irregular galaxy in orbit around our own Milky Way. It is a large object, several degrees in size, and easily visible to the unaided eye in Southern Hemisphere skies. The LMC is located in the constellation of Doradus at about 5h30m Right Ascension, -68 degrees Declination, and lies at a distance of roughly 50 kiloparsecs (160,000 light years) from Earth. ...

Тема : Nubecula Minor (Cape Clouds) - Малое Магелланово Облако (Small Magellanic Cloud), карликовая галактика NGC 292 в созвездии Тукан (Tucana) .. ... Nubecula Minor (Cape Clouds) - Малое Магелланово Облако (Small Magellanic Cloud), карликовая галактика NGC 292 в созвездии Тукан (Tucana) .. ... Малое Магелланово Облако (Small Magellanic Cloud, NGC 292) .: . ... Как найти Малое Магелланово Облако (Small Magellanic Cloud, NGC 292)? ... NGC 292, Small Magellanic Cloud (SMC), Малое Магелланово Облако .. ...

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... GSAOI Home . ... Science . ... Despite vast increase in our understanding of the evolutionary nature of planetary nebulae (PNe) during the last three decades, a central question remains: where is the missing mass? Theoretical evolutionary tracks predict that all stars with masses in the range 1.4-8 M Sun should become PNe. ... Clearly, much of the mass of the planetary nebula shell must remain un-ionized, and much of it may be in molecular form. ... The Magellanic Cloud PNe are ideal for this. ...

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. Home . News . Gallery . Events . Twitter . Press Releases . Links . Contact Us . Calendar . Press & Web Coverage . Next . List . The season for noctilucent clouds is not over yet! . More noctilucent coulds photos from Jonathan Bingham: . "I took these at 02.45 on the morning of Saturday 25 July; a bright display aprox 20' across and 10' high. It really caught one's attention." . Monday, 27 July 2009 09:46 . International Year of Astronomy, Ireland National Node . [Back To Top] .

... Operating at a wavelength of 10 ?m, it produces a 135њx135њ image with a resolution of 0.9њ. ... The clouds move from the west-southwest. ... At the same time as the IR images, visible light images were taken with an Apple Computer QuickTake electronic camera. ... At 1540 MDT, the large central cloud is visible in both images. At 1544 MDT, a distinctive cloud is apparent near the center in the visible image and right of center in the IR. The performance of the SDSS cloud scanner is excellent. ...

... Галактика - SB(s)m pec . ... Малое Магелланово Облако вместе с соседним с ним Большим Магеллановым Облаком - БМО (Large Magellanic Cloud - LMC) - выдающиеся небесные объекты южного полушария, прекрасно видимые невооруженным взглядом. ... ММО является третьей по близости к Млечному Пути галактикой после Sagittarius Dwarf Elliptical Galaxy и БМО . ... Скопление NGC121 в ММО состоит из звезд, возраст которых сравним с возрастом старейших шаровых скоплений из гало нашей Галактики. ...

... The spectrum of the Sgr B2 molecular cloud has been surveyed between 215 and 265 GHz towards 3 positions, the dense cores Sgr B2(N)and Sgr B2(M), and the quiescent core Sgr B2(NW). ... The Sgr B2 molecular cloud, located approximately 100 pc from the Galactic Centre and with a mass of , is one of the most extreme cases among star formation sites ( Lis & Goldsmith (1991) ). ... Of the 3 observed positions Sgr B2(N) has the strongest line emission in most molecular species with a few exceptions. ...

Next: Computation of the Up: Typical Run Previous: Edition of the . This table is used both as an input and output by the main program. The table content is: . INPUT . Parameters relative to the absorption lines . ... OUTPUT . In output, the program will write in this table, for each absorption line, the velocity of the corresponding cloud relative to the source and its redshift (relative to the observer). A template of this table can be found in MID_CLOUD:ABSC.TBL . ...

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... HyperXR Cloud имеет сверхмягкое оголовье, амбушюры с памятью формы и чашки из искусственной кожи для комфортной игры в любое время. Гарнитура предлагается по доступной цене, поэтому также не станет причиной головной боли. HyperX Cloud оптимизирована для про-гейминга и обеспечивает яркое звучание с кристально чистыми низкими, средними и высокими частотами, а также улучшенную передачу басов, позволяющую полностью насладиться победой. ...

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