Explanation: A satellite galaxy of the Milky Way, the Small Magellanic Cloud (SMC) is a wonder of the southern sky, a mere 210,000 light-years distant in the constellation Tucana. Found among the SMC's clusters and nebulae NGC 346 is a star forming region about 200 light-years across, pictured above by the Hubble Space Telescope. Exploring NGC 346, astronomers have identified a population of embryonic stars strung along the dark, intersecting dust lanes visible here on the right. Still collapsing within their natal clouds, the stellar infants' light is reddened by the intervening dust. A small, irregular galaxy, the SMC itself represents a type of galaxy more common in the early Universe. But these small galaxies are thought to be a building blocks for the larger galaxies present today. Within the SMC, stellar nurseries like NGC 346 are also thought to be similar to those found in the early Universe.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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NASA Official: Jay Norris. Specific rights apply.
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& Michigan Tech. U.

Publikacii s klyuchevymi slovami: NGC 346 - star formation - SMC - zvezdoobrazovanie - Maloe Magellanovo Oblako Publikacii so slovami: NGC 346 - star formation - SMC - zvezdoobrazovanie - Maloe Magellanovo Oblako
Sm. takzhe: IC 348 i Barnard 3 NGC 602: zvezdy protiv stolbov M16: stolpy sozidaniya Zvezdnaya fabrika Mess'e 17 IC 5146: tumannost' Kokon Kometarnye globuly NGC 602: zvezdnoe skoplenie Ustrica Vse publikacii na tu zhe temu >>