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You entered: diffuse emission
![Голубая лагуна](https://images.astronet.ru/pubd/2006/08/25/0001215423/lagoon_croman_nostars.preview.jpg)
25.08.2006
Stars come and go as you slide your cursor over this engaging image of M8, aka the Lagoon Nebula. Of course, the nebula is itself a star-forming region, but the stars that appear and disappear here include background and foreground stars that by chance lie along the same line of sight.
![Загадочная туманность Конус](https://images.astronet.ru/pubd/2002/01/07/0001174010/cone_gendler.preview.jpg)
7.01.2002
Sometimes the simplest shapes are the hardest to explain. For example, the origin of the mysterious cone-shaped region seen on the far left remains a mystery. The interstellar formation, dubbed the Cone Nebula, is located about 2700 light years away.
![Загадочная туманность Конус](https://images.astronet.ru/pubd/2005/12/26/0001210614/cone_gabany.preview.jpg)
25.12.2005
Sometimes the simplest shapes are the hardest to explain. For example, the origin of the mysterious cone-shaped region seen on the far left remains a mystery. The interstellar formation, dubbed the Cone Nebula, is located about 2700 light years away.
![Глубокое поле Розетки](https://images.astronet.ru/pubd/2024/02/14/0001920571/RosetteCone_Bernard_960.preview.jpg)
14.02.2024
Can you find the Rosette Nebula? The large, red, and flowery-looking nebula on the upper left may seem the obvious choice, but that is actually just diffuse hydrogen emission surrounding the Cone and Fox Fur Nebulas.
![Из чего сделана Туманность Омега](https://images.astronet.ru/pubd/2001/01/06/0001164889/omega_sqiid_big.preview.jpg)
11.12.2000
The Omega Nebula is a massive, complex cloud of dust and gas from which new stars are continually forming. The similarity to the Greek letter capital Omega gives the molecular cloud its popular name, but the nebula is also known as the Swan Nebula, the Horseshoe Nebula, and M17.
![Скопления в центре Галактики](https://images.astronet.ru/pubd/2006/08/10/0001215162/gcenter_cxc_c.preview.jpg)
10.08.2006
If you had x-ray vision, the central regions of our Galaxy would not be hidden from view by cosmic dust clouds. Instead, the Milky Way toward Sagittarius might look something like this. Pleasing...
![Излучение и отражение в NGC 6559](https://images.astronet.ru/pubd/2001/10/24/0001171912/ngc6559_gendler.preview.jpg)
23.10.2001
Bright gas and dark dust permeate the space between stars in a nebula known as NGC 6559. The gas, primarily hydrogen, is responsible for the diffuse red glow of the emission nebula. As energetic...
![Горячее газовое гало вокруг галактики NGC 4631](https://images.astronet.ru/pubd/2002/08/25/0001179299/ngc4631_chandra.preview.jpg)
25.07.2001
Is our Milky Way Galaxy surrounded by a halo of hot gas? A step toward solving this long-standing mystery was taken recently with Chandra X-ray observations of nearby galaxy NGC 4631. In the above composite picture, newly resolved diffuse X-ray emission is shown in blue, superposed on a HST image showing massive stars in red.
![NGC 281: скопление, облака и глобулы](https://images.astronet.ru/pubd/2004/10/20/0001200470/ngc281_sauer.preview.jpg)
20.10.2004
NGC 281 is a busy workshop of star formation. Prominent features include a small open cluster of stars, a diffuse red-glowing emission nebula, large lanes of obscuring gas and dust, and dense knots of dust and gas in which stars may still be forming.
![NGC 281: туманность Пэкмен](https://images.astronet.ru/pubd/2005/08/23/0001207695/pacman_cannistra.preview.jpg)
23.08.2005
NGC 281 is a busy workshop of star formation. Prominent features include a small open cluster of stars, a diffuse red-glowing emission nebula, large lanes of obscuring gas and dust, and dense knots of dust and gas in which stars may still be forming.
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