HubbleSite - Picture Album: Star Cluster NGC 2074 in the Large Magellanic Cloud
HubbleSite - Picture Album: Taken Under the �Wing� of the Small Magellanic Cloud
Astronomy Picture of the Day: 01/18/14 - Dancing Squid This is NGC 1760 (also known as N11 or the Dancing Squid nebula), one of the most massive, active star-forming regions located in our local corner of the universe. More specifically, this region belongs to the northern part of a neighboring dwarf-galaxy of the Milky Way; a little place you may know of as the Large Magellanic Cloud. The intricate network of interlinking cosmic 'bubbles' extend about 1,000 lig
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It's the bubble versus the cloud. NGC 7635, the Bubble Nebula, is being pushed out by the stellar wind of massive central star BD+602522.
Star-forming region NGC 3603 (Milky Way), about 20,000 ly away, contains a massive young star cluster, formed in a huge rush of star formation thought to have occurred about 1 Ma
-- NGC 7822: a young star-forming region in Cepheus -- 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, the glowing star forming region lies about 3,000 light-years away. - Image Credit: Manuel Fernández Suarez - Image enhancement: Jean-Baptiste Faure
Amazing Space Photos ~ Pacman Nebula In visible light, the star-forming cloud known as NGC 281 in the constellation of Cassiopeia appears
The Butterfly Nebula - NGC 6302 (also called the Bug Nebula, Butterfly Nebula, or Caldwell 69) is a bipolar planetary nebula in the constellation Scorpius. The structure in the nebula is among the most complex ever observed in planetary nebulae. The spectrum of NGC 6302 shows that its central star is one of the hottest stars in the galaxy, with a surface temperature in excess of 200,000 K, implying that the star from which it formed must have been very large.
A Halo for NGC 6164. Beautiful emission nebula NGC 6164 was created by a rare, hot, luminous O-type star, some 40 times as massive as the
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