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
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Starburst Cluster NGC 1929 in the Large Magellanic Cloud This cluster is creating shockwave “superbubbles” that are triggering chain reactions of supernova explosions. This image is a composite of three light wavelengths, X-rays are represented as blue, visible light as yellow, and infra-red light as red.
NGC 2818 It may look like a seahorse, but the dark object is actually a pillar of smoky dust about 20 light-years long. The structure occurs in our neighbouring Large Magellanic Cloud, in a star-forming region near the Tarantula Nebula.
Hubble images remarkable double cluster located in the Large Magellanic Cloud. Credit: ESA, NASA and Martino Romaniello (European Southern Observatory, Germany)
NGC 602 is a young, bright open cluster of stars located in the Small Magellanic Cloud (SMC), a satellite galaxy to the Milky Way. Radiation and shock waves from the stars have pushed away much of the lighter surrounding gas and dust that compose the nebula known as N90, and this in turn has triggered new star formation in the ridges (or "elephant trunks") of the nebula.
The star cluster Pismis 24 lies in the core of the large emission nebula NGC 6357 that extends one degree on the sky in the direction of the Scorpius constellation. Part of the nebula is ionised by the youngest (bluest) heavy stars in Pismis 24. The intense ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder.
region of star cluster NGC 6611, from The Celestial Handbook, by Robert Burnham Jr., 1966
A Halo for NGC 6164 Image Credit & Copyright: Don Goldman Explanation: Beautiful emission nebula NGC 6164 was created by a rare, hot, luminous O-type star, some 40 times as massive as the Sun. Seen at the center of the cosmic cloud, the star is a mere 3 to 4 million years old. In another three to four million years the massive star will end its life in a supernova explosion. Spanning around 4 light-years, the nebula itself has a bipolar symmetry.
Amazing Space Photos ~ Pacman Nebula In visible light, the star-forming cloud known as NGC 281 in the constellation of Cassiopeia appears
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This photo, released by NASA and the European Space Agency to commemorate the Hubble Space Telescope’s completion of 100,000th orbit around the Earth in its 18th year of exploration and discovery, scientists have aimed Hubble to take a snapshot of a dazzling region of celestial birth and renewal. In the image, a small portion of the nebula star cluster NGC 2074, located 170,000 light-years away, can be observed.
-- 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
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#Hodge301 is a star cluster located in the #TarantulaNebula about 168,000 light years away in the Large Magellanic Cloud Galaxy. The Tarantula Nebula is a star forming region, fueled by the star clusters hidden inside. The stars of Hodge 301 formed tens of millions of years ago. The most massive quickly ran through their fuel and erupted into supernovae.
Young Stars Sculpt Gas with Powerful Outflows in the Small Magellanic Cloud
Once thought to be part of the Orion nebula, the star cluster NGC 1980 is actually a separate entity, scientists say. It appears around the brightest star seen at the bottom of this image, iota Ori. The disks around the star are the result of internal light reflection in the camera optics.
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Cotton Candy Nebula - The nebula known as N11, complete with sparkly star clusters embedded in fluffy pink clouds of gas. This exceptionally energetic star-forming region, also known as the Bean Nebula, extends over 1,000 light-years in the Large Magellanic Cloud. Three generations of star formation have created shells of gas and dust which are being blown away by radiation from the newborn stars.
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.
NGC 6193 & NGC 6188 (Curtis-Schmidt telescope at Cerro Tololo Inter-American Ob. Chile). NGC 6188 is an emission nebula located about 4000 ly away in the constel. Ara. The bright open cluster NGC 6193 is responsible for a region of reflection nebulosity w/in NGC6188Nebula of Stars and Colorful Gas - Long, Tall, Vertical Pins