Explanation: The massive stars of NGC 346 are short lived, but very energetic. The star cluster is embedded in the largest star forming region in the Small Magellanic Cloud, some 210,000 light-years distant. Their winds and radiation sweep out an interstellar cavern in the gas and dust cloud about 200 light-years across, triggering star formation and sculpting the region's dense inner edge. Cataloged as N66, the star forming region also appears to contain a large population of infant stars. A mere 3 to 5 million years old and not yet burning hydrogen in their cores,the infant stars are strewn about the embedded star cluster. In the above false-color Hubble Space Telescope image, visible and near-infrared light are seen as blue and green, while light from atomic hydrogen emission is red.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: NGC 346 - star formation - star cluster - zvezdoobrazovanie - zvezdnoe skoplenie Publikacii so slovami: NGC 346 - star formation - star cluster - zvezdoobrazovanie - zvezdnoe skoplenie
Sm. takzhe: IC 348 i Barnard 3 M16: stolpy sozidaniya Molodoe zvezdnoe skoplenie NGC 1333 Zvezdnaya fabrika Mess'e 17 IC 5146: tumannost' Kokon Kometarnye globuly Vybrosy iz protozvezd v Zmee Vse publikacii na tu zhe temu >>