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Planetarnaya tumannost' Krasnyi Pauk
<< Vchera 6.01.1998 Zavtra >>
Planetarnaya tumannost' Krasnyi Pauk
Avtory i prava: B. Balik ( universitet v Vashingtone ) i dr., Shirokougol'naya planetnaya kamera 2 , kosmicheskii teleskop im. Habbla , NASA
Poyasnenie: Kakuyu zaputannuyu pautinu mozhet splesti planetarnaya tumannost' . Slozhnaya struktura planetarnoi tumannosti Krasnyi Pauk obrazovalas' v rezul'tate vybrosa iz obychnoi zvezdy vneshnih gazovyh obolochek i prevrasheniya ee v belyi karlik . Eta simmetrichnaya tumannost' s dvumya ushami, oboznachaemaya takzhe NGC 6537, soderzhit samyi goryachii belyi karlik . Etot belyi karlik vozmozhno yavlyaetsya chast'yu dvoinoi zvezdnoi sistemy . Vnutrennie vetry , duyushie iz central'nyh zvezd, pokazany v central'noi vstavke na etoi kartinke i imeyut skorost' 300 km v sekundu. Eti vetry zastavlyayut tumannost' rasshiryat'sya, chto privodit k stolknoveniyu gaza i pyli. Atomy stalkivayushegosya veshestva izluchayut harakternyi svet.

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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.

English text
Po materialam Astronomy Picture Of the Day
Publikacii s klyuchevymi slovami: planetary nebula - belyi karlik - Planetarnaya tumannost'
Publikacii so slovami: planetary nebula - belyi karlik - Planetarnaya tumannost'
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