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Keywords: LMC, Tarantula Nebula, star formation
![Выбросы из протозвезд в Змее](https://images.astronet.ru/pubd/2024/06/27/0001931781/STScI-SerpNorth1024.preview.png)
27.06.2024
Jets of material blasting from newborn stars, are captured in this James Webb Space Telescope close-up of the Serpens Nebula. The powerful protostellar outflows are bipolar, twin jets spewing in opposite directions. Their directions are perpendicular to accretion disks formed around the spinning, collapsing stellar infants.
![Звездное скопление R136](https://images.astronet.ru/pubd/2007/05/07/0001221916/r136_hst.preview.jpg)
6.05.2007
In the center of star-forming region 30 Doradus lies a huge cluster of the largest, hottest, most massive stars known. These stars, known as the star cluster R136, and part of the surrounding nebula are captured here in this gorgeous visible-light image from the Hubble Space Telescope.
![Темная туманность Линдса LDN1251](https://images.astronet.ru/pubd/2020/07/04/0001674343/ldn1251_jerahian1024.preview.jpg)
3.07.2020
Stars are forming in Lynds Dark Nebula (LDN) 1251. About 1,000 light-years away and drifting above the plane of our Milky Way galaxy, the dusty molecular cloud is part of a complex of dark nebulae mapped toward the Cepheus flare region.
![Темная туманность Линдса LDN 1251](https://images.astronet.ru/pubd/2022/11/24/0001858531/LDN1251v7social1024.preview.png)
24.11.2022
Stars are forming in Lynds Dark Nebula (LDN) 1251. About 1,000 light-years away and drifting above the plane of our Milky Way galaxy, the dusty molecular cloud is part of a complex of dark nebulae mapped toward the Cepheus flare region.
![Первый взгляд XMM-Ньютон: рентгеновские лучи от Большого Магелланова Облака](https://images.astronet.ru/pubd/2006/11/10/0001217536/lmc30dor_xmmpn_big.preview.jpg)
11.02.2000
Recently the European Space Agency released this and other spectacular "first light" pictures from its new orbiting x-ray observatory, christened XMM-Newton. A churning region of star birth and death in our small neighboring galaxy, the Large Magellanic Cloud (LMC), this field was one of several chosen to test out XMM-Newton's x-ray imaging capabilities.
![Звездные лаборатории в Большом Магеллановом Облаке](https://images.astronet.ru/pubd/2003/08/14/0001192294/lmc2_um.preview.jpg)
25.07.1997
Stars are evolving in the Large Magellanic Clouds (LMC). This is particularly evident in the above close-up of the LMC's edge, which appears about as large as the full moon. Visible only...
![Хенице 70: очень большой пузырь в Большом Магеллановом Облаке](https://images.astronet.ru/pubd/2002/08/26/0001179336/henize70_aat.preview.gif)
10.05.1996
Massive stars (tens of times the mass of the Sun) profoundly affect their galactic environment. Churning and mixing the clouds of gas and dust between the stars, they leave their mark in the compositions and locations of future generations of stars and star systems.
![Бурная активность остатка сверхновой N63A](https://images.astronet.ru/pubd/2005/06/08/0001206192/n63a_hst.preview.jpg)
8.06.2005
What has this supernova left behind? As little as 2,000 years ago, light from a massive stellar explosion in the Large Magellanic Clouds (LMC) first reached planet Earth. The LMC is a close...
![Светящийся газ в галактике БМО](https://images.astronet.ru/pubd/2006/01/23/0001211048/lmcgas_ctio.preview.jpg)
23.01.2006
What goes on inside of a galaxy? To help find out, astronomers from the Magellanic Cloud Emission Line Survey team imaged our neighboring LMC galaxy in spectacular detail and highlighted very specific colors of light emitted by glowing gas.
![IC 1805: туманность Сердце](https://images.astronet.ru/pubd/2009/02/16/0001233414/IC1805_Daniel_rc800.preview.jpg)
14.02.2009
Sprawling across almost 200 light-years, emission nebula IC 1805 is a mix of glowing interstellar gas and dark dust clouds. Derived from its Valentine's-Day-approved shape, its nickname is the Heart Nebula. About 7,500 light-years away in the Perseus spiral arm of our galaxy, stars were born in IC 1805.
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