Poyasnenie: Bol'shaya zvezdnaya associaciya, zanesennaya v katalog kak NGC 206, raspolozhilas' v bogatyh pyl'yu rukavah sosednei spiral'noi galaktiki Andromedy (M31), udalennoi na 2.5 millionov svetovyh let. Yarkie golubye zvezdy NGC 206 svidetel'stvuyut o ee molodosti. Oni vidny okolo centra etogo chetkogo vida krupnym planom na yugo-zapadnuyu chast' diska galaktiki Andromedy. Vozrast samyh molodyh massivnyh zvezd men'she 10 millionov let. Razmer NGC 206 – okolo 4 tysyach svetovyh let, ona namnogo bol'she skoplenii molodyh zvezd v diske nashego Mlechnogo Puti, izvestnyh kak rasseyannye ili galakticheskie skopleniya. Primerno takoi razmer imeyut gigantskie zvezdnye yasli NGC 604 v blizkoi spiral'noi galaktike M33 i tumannost' Tarantul v Bol'shom Magellanovom Oblake.

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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.
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& Michigan Tech. U.

Publikacii s klyuchevymi slovami: M 31 - Andromeda galaxy - Tumannost' Andromedy Publikacii so slovami: M 31 - Andromeda galaxy - Tumannost' Andromedy
Sm. takzhe: M31: galaktika Andromedy Andromeda nad Al'pami Zvezdy Andromedy: nastoyashee i budushee Meteor i galaktika NGC 206 i zvezdnye oblaka Andromedy Neozhidannye oblaka v napravlenii na galaktiku Andromedy Oblaka vokrug galaktiki Andromedy Vse publikacii na tu zhe temu >>