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Oblako Klyaimana-Lou
<< Vchera 2.03.1999 Zavtra >>
Oblako Klyaimana-Lou
Avtory i prava: Ohlazhdaemyi infrakrasnyi spektrometr i kamera , 8.3-m teleskop Subaru , Nacional'naya astronomicheskaya observatoriya Yaponii
Perevod: kozyreva, Timoshenko A.D.
Poyasnenie: Samoi aktivnoi oblast'yu v komplekse tumannosti Oriona yavlyaetsya oblako Klyaimana-Lou. V nei skoplenie molodyh i formiruyushihsya zvezd vkrapleno v molekulyarnoe oblako, soderzhashee bol'shoe kolichestvo pyli. Pyl' v znachitel'noi stepeni pogloshaet vidimoe izluchenie ot oblaka Klyaimana-Lou, odnako v infrakrasnom diapazone, kak pokazano na segodnyashnei kartinke, oblako bukval'no vzryvaetsya kraskami. Massivnye molodye zvezdy oblaka Klyaimana-Lou vyduvayut goryachii zvezdnyi veter - pronizyvayushii i nagrevayushii okruzhayushii gaz, tak chto obrazuyutsya pal'ceobraznye struktury. Okolo centra oblaka Klyaimana-Lou raspolozhena chrezvychaino aktivnaya zvezda IRc2, massa kotoroi ocenivaetsya v 30 mass Solnca. Nedavnie radionablyudeniya pokazali, chto v oblake Klyaina-Lou nahodyatsya ispuskayushie moshnoe izluchenie vodyanye mazery.

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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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English text
Po materialam Astronomy Picture Of the Day
Publikacii s klyuchevymi slovami: nebula - molecular cloud - tumannost'
Publikacii so slovami: nebula - molecular cloud - tumannost'
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