News on interstellar matter
- Cygnus-X: the cool swan glowing in flight
- New molecules and star formation in the Milkyway
- The dust in the belt of Orion
- Missing dark matter in interstellar space around the Sun
- New 15meter telescope first ligth
- Tiny particles key to understanding early solar system
- New WISE catalog of entire infrared sky
- The Milkyway is full of bubbles
- Discovery of solid buckyballs in space
- Sources of rare Earth-elements found in space
- Dark clouds in Taurus
- Alien matter in the Solar system
- New mapping show cold gas and strange haze
- The sound of the universe
- Discovery of million degrees hot molecular gasses
- Most detailed infrared image of the Carina nebula
- An interstellar star-nursery
- Infrared image of the famous Helix-nebula
- Widefield infrared view of Milkyway's dust
- The smoky core of the Omega Nebula M17
- Star rebels against its parent cloud
- Observation of a cool gas-cloud being swallowed by black hole
- European astronomers discover cocoons of radiation in nebula
- SOFIA airborne observatory views star forming region W40
- The Cool Clouds of the Carina-nebula
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Interstellar bubbles
Wednesday, 13 April 2011 11:55
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| Astronomy - Interstellar matter |
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This image of the nebula NGC 3582 shows giant loops of gas bearing a striking resemblance to solar prominences. These loops are thought to have been ejected by dying stars, but new stars are also being born, emitting intense UV-radiation that makes the gas in the nebula glow, producing the fiery display shown here. The image of the nebula NGC 3582 was captured by the Wide Field Imager on the MPG/ESO 2,2metre telescope at ESO’s La Silla Observatory in Chile NGC 3582 is part of a large star-forming region in the Milky Way, called RCW 57. It lies close to the central plane of the Milky Way in the southern constellation of Carina (The Keel of Jason’s ship, the Argo). John Herschel first saw this complex region of glowing gas and dark dust clouds in 1834, during his stay in South Africa. Some of the stars forming in regions like NGC 3582 are much heavier than the Sun. These monster stars emit energy at prodigious rates and have very short lives that end in explosions as supernovae. The material ejected from these dramatic events creates bubbles in the surrounding gas and dust. This is the probable cause of the loops visible in this picture. (Image Courtsey ESO. Click for full resolution) This image was taken through multiple filters. From the Wide Field Imager, data taken through a red filter are shown in green and red, and data taken through a filter that isolates the red glow characteristic of hydrogen are also shown in red. Additional infrared data from the Digitized Sky Survey are shown in blue. The image was processed by ESO using the observational data identified by Joe DePasquale, from the United States, who participated in ESO’s Hidden Treasures 2010 astrophotography competition. The competition was organised by ESO in October–November 2010, for everyone who enjoys making beautiful images of the night sky using astronomical data obtained using professional telescopes. Joe searched through ESO’s archive and identified datasets that he used to compose his image of NGC 3582, which was the tenth highest ranked entry in the competition, out of almost 100 entries. His original work can be seen here. Source: ESO |




