Poyasnenie: Kogda zvezda tipa Solnca bol'she ne v sostoyanii podderzhivat' termoyadernye reakcii v yadre, ee centr szhimaetsya v belyi karlik, a vneshnie sloi zvezdnoi atmosfery vybrasyvayutsya v mezhzvezdnoe prostranstvo i prevrashayutsya v planetarnuyu tumannost'. Vy vidite planetarnuyu tumannost' s ochen' strannoi i haotichnoi strukturoi. Vnutrennyaya chast' tumannosti soderzhit neobychnoe rasshiryayusheesya gazovoe kol'co. My ego vidim pochti s rebra. Tochnyi mehanizm, kotoryi vyduvaet gaz planetarnoi tumannosti, do konca neyasen, a poetomu ostaetsya predmetom astronomicheskih issledovanii.

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

Publikacii s klyuchevymi slovami: planetary nebula - Evolyuciya zvezd - Planetarnaya tumannost' - belyi karlik Publikacii so slovami: planetary nebula - Evolyuciya zvezd - Planetarnaya tumannost' - belyi karlik
Sm. takzhe: M27: eto ne kometa Dzhons-Emberson-1 Kol'ca vokrug tumannosti Kol'co HFG1 i Eibell 6: planetarnye tumannosti NGC 2440: kokon novogo belogo karlika MyCn 18: planetarnaya tumannost' Pesochnye Chasy Tumannost' Kol'co ot teleskopa "Dzheims Vebb" Vse publikacii na tu zhe temu >>