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Keywords: gamma-ray burst, star formation, afterglow, hypernova
![Массивные звезды в NGC 6357](https://images.astronet.ru/pubd/2016/02/05/0001355700/NGC6357schedler_S2HaO3_25.preview.jpg)
5.02.2016
Massive stars lie within NGC 6357, an expansive emission nebula complex some 6,500 light-years away toward the tail of the constellation Scorpius. In fact, positioned near center in this ground-based close-up...
![M16: столпы созидания](https://images.astronet.ru/pubd/2016/04/24/0001361254/pillars7_hst_960.preview.jpg)
24.04.2016
Newborn stars are forming in the Eagle Nebula. This image, taken with the Hubble Space Telescope in 1995, shows evaporating gaseous globules (EGGs) emerging from pillars of molecular hydrogen gas and dust. The giant pillars are light years in length and are so dense that interior gas contracts gravitationally to form stars.
![Область звездообразования S106](https://images.astronet.ru/pubd/2016/02/16/0001356616/S106_Pimenta_960.preview.jpg)
16.02.2016
Massive star IRS 4 is beginning to spread its wings. Born only about 100,000 years ago, material streaming out from this newborn star has formed the nebula dubbed Sharpless 2-106 Nebula (S106), featured here.
![Звёзды и пылевые столбы в NGC 7822 от WISE](https://images.astronet.ru/pubd/2014/12/01/0001326873/ngc7822_WISEantonucci_1080c.preview.jpg)
30.11.2014
Hot, young stars and cosmic pillars of gas and dust seem to crowd into NGC 7822. At the edge of a giant molecular cloud toward the northern constellation Cepheus, this glowing star forming region lies about 3,000 light-years away.
![Звездообразование в туманности Головастик](https://images.astronet.ru/pubd/2014/11/20/0001326100/ic410_WISEantonucci_960.preview.jpg)
17.11.2014
Dusty emission in the Tadpole nebula, IC 410, lies about 12,000 light-years away in the northern constellation Auriga. The cloud of glowing gas is over 100 light-years across, sculpted by stellar winds and radiation from embedded open star cluster NGC 1893.
![Желтые шары в W33](https://images.astronet.ru/pubd/2015/02/02/0001331773/sig15-02spitzerW331066.preview.jpg)
30.01.2015
Infrared wavelengths of 3.6, 8.0, and 24.0 microns observed by the Spitzer Space Telescope are mapped into visible colors red, green, and blue in this striking image. The cosmic cloud of gas and dust is W33, a massive starforming complex some 13,000 light-years distant, near the plane of our Milky Way Galaxy.
![Широкое поле с ρ Змееносца](https://images.astronet.ru/pubd/2014/07/27/0001318163/RhoOphWide_andreo_960.preview.jpg)
27.07.2014
The clouds surrounding the star system Rho Ophiuchi compose one of the closest star forming regions. Rho Ophiuchi itself is a binary star system visible in the light-colored region on the image right.
![Цветные звёздные облака в Лебеде](https://images.astronet.ru/pubd/2015/04/22/0001336016/barnard344_vanderHoeven_960.preview.jpg)
22.04.2015
Stars can form in colorful surroundings. Featured here is a star forming region rich in glowing gas and dark dust toward the constellation of the Swan (Cygnus), near the bright star Sadr. This region, which spans about 50 light years, is part of the Gamma Cygni nebula which lies about 1,800 light years distant.
![Скопление Мелотт 15 в туманности Сердце](https://images.astronet.ru/pubd/2014/10/19/0001323796/ic1805nb_eder1024.preview.jpg)
18.10.2014
Cosmic clouds form fantastic shapes in the central regions of emission nebula IC 1805. The clouds are sculpted by stellar winds and radiation from massive hot stars in the nebula's newborn star cluster, Melotte 15.
![В глубине Лагуны](https://images.astronet.ru/pubd/2015/07/29/0001339260/block_m8_32ins1024.preview.jpg)
29.07.2015
Ridges of glowing interstellar gas and dark dust clouds inhabit the turbulent, cosmic depths of the Lagoon Nebula. Also known as M8, The bright star forming region is about 5,000 light-years distant.
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