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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Hubble images remarkable double cluster located in the Large Magellanic Cloud. Credit: ESA, NASA and Martino Romaniello (European Southern Observatory, Germany)
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.
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.
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Star Cluster NGC 3532 – A Colorful Gathering of Middle-Aged Stars 11/26/14 The MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile captured this richly colorful view of the bright star cluster NGC 3532.
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.
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.
region of star cluster NGC 6611, from The Celestial Handbook, by Robert Burnham Jr., 1966
Amazing Space Photos ~ Pacman Nebula In visible light, the star-forming cloud known as NGC 281 in the constellation of Cassiopeia appears
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.
#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
At the center of Messier 80, a globular star cluster in Scorpius-Messier 80 (NGC 6093) is a globular star cluster with a diameter of approximately 95 light-years, about 32,600 light-yrs away in the constellation Scorpius.
-- 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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Hubble Space Telescope image of the R136 super star cluster, near the center of the 30 Doradus Nebula, also known as the Tarantula Nebula or NGC 2070.
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.
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.
Stellar cluster NGC 2467 and its surrounds, located in the constellation Puppis ("The Stern"). A few million years old at most, it is a very active stellar nursery, where new stars are born continuously from large clouds of dust and gas. The image contains open clusters Haffner 18 (center) & Haffner 19 (middle right) and vast areas of ionised gas. The bright star at the center of the largest pink region is HD 64315, a massive young star helping to shape the structure of the whole nebular region.