![]() |
Keywords: H-alpha, pulsar, supernova remnant
![Остаток сверхновой Кеплера в рентгеновских лучах](https://images.astronet.ru/pubd/2007/01/16/0001220314/keplersnr_chandra.preview.jpg)
16.01.2007
What caused this mess? Some type of star exploded to create the unusually shaped nebula known as Kepler's supernova remnant, but which type? Light from the stellar explosion that created this energized cosmic cloud was first seen on planet Earth in October 1604, a mere four hundred years ago.
![N132D и цвет рентгеновских лучей](https://images.astronet.ru/pubd/2002/05/23/0001177038/n132d_cxc_xraycolor_c1.preview.jpg)
23.05.2002
Supernova remnant N132D shows off complex structures in this sharp, color x-ray image. Still, overall this cosmic debris from a massive star's explosive death has a strikingly simple horseshoe shape. While N132D lies 180,000 light-years distant in the Large Magellanic Cloud, the expanding remnant appears here about 80 light-years across.
![Туманность Вуаль](https://images.astronet.ru/pubd/2010/09/16/0001247117/Veil_pugh_900c.preview.jpg)
16.09.2010
Delicate in appearance, these filaments of shocked, glowing gas, draped in planet Earth's sky toward the constellation of Cygnus, make up the Veil Nebula. The nebula is a large supernova remnant, an expanding cloud born of the death explosion of a massive star.
![Исчезающая туманность Медуза](https://images.astronet.ru/pubd/2010/05/17/0001245087/ic443_franke900.preview.jpg)
15.05.2010
Normally faint and elusive, the Jellyfish Nebula is caught in this alluring, false-color, telescopic view. Flanked by two bright stars, Mu and Eta Geminorum, at the foot of a celestial twin, the Jellyfish Nebula is the brighter arcing ridge of emission with dangling tentacles below and right of center.
![Симеиз 147: остаток сверхновой](https://images.astronet.ru/pubd/2002/08/30/0001179464/s147_mandel.preview.jpg)
30.08.2002
It's easy to get lost following the intricate filaments in this stunningly detailed image of faint supernova remnant Simeis 147. Seen towards the constellation Taurus it covers nearly 3 degrees (6 full moons)...
![Симеиз 147: остаток сверхновой](https://images.astronet.ru/pubd/2005/03/24/0001204938/s147_gendler_full.pr.jpg)
24.03.2005
It's easy to get lost following the intricate filaments in this detailed image of faint supernova remnant Simeis 147. Seen towards the constellation Taurus it covers nearly 3 degrees (6 full moons) on the sky corresponding to a width of 150 light-years at the stellar debris cloud's estimated distance of 3,000 light-years.
![Газовая пуля из космического взрыва N49](https://images.astronet.ru/pubd/2010/07/01/0001245785/n49_chandra.preview.jpg)
30.06.2010
What is that strange blue blob on the far right? No one is sure, but it might be a speeding remnant of a powerful supernova that was unexpectedly lopsided. Scattered debris from supernova explosion N49 lights up the sky in this gorgeous composited image based on data from the Chandra and Hubble Space Telescopes.
![Водород в M33](https://images.astronet.ru/pubd/2006/11/23/0001218011/m33hargb_schur_F717.preview.jpg)
23.11.2006
Gorgeous spiral galaxy M33 seems to have more than its fair share of hydrogen. Its inner 30,000 light-years are shown here in an image processed to fully reveal the reddish glow of ionized hydrogen regions (HII regions) sprawling along loose spiral arms as they wind toward the galaxy's core.
![Туманности в Лебеде](https://images.astronet.ru/pubd/2003/10/23/0001194333/cygnusha_mandel_c3.preview.jpg)
23.10.2003
Looking toward the constellation Cygnus, a stunning and complex region of nebulae strewn along the plane of our Milky Way galaxy is revealed in this unique wide-angle sky view. Recorded with a filter designed...
![Бурлящее оранжевое Солнце](https://images.astronet.ru/pubd/2010/06/09/0001245437/orangesun_friedman.preview.jpg)
9.06.2010
Even a quiet Sun can be a busy place. And over the deep Solar Minimum of the past few years, our Sun has been unusually quiet. The above image, taken last week...
|
January February March April May June |