File:HE 0437-5439 mechanism.jpg

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Description
English: This illustration shows one possible mechanism for how the star HE 0437-5439 acquired enough energy to be ejected from our Milky Way galaxy.
Українська: Еволюція потрійної зоряної системи HE 0437-5439 до однієї зорі із набуттям прискорення та вильотом за межі нашої Галактики.
Русский: Звезда изначально входила в состав тройной звездной системы, которая порядка 100 миллионов лет назад вращалась вокруг центра Млечного пути. Однако на одном из этапов своего существования звездное трио слишком близко подошло к сверхмассивной черной дыре, находящейся в центре Млечного пути, и в результате одна из звезд была "съедена" черной дырой, две других - выброшены со своих орбит. После грандиозного воздействия две звезды слились в единую существующую и поныне.
Date
Source http://hubblesite.org/newscenter/archive/releases/2010/19/image/c/
Author NASA, ESA, O. Gnedin (University of Michigan, Ann Arbor), and W. Brown (Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass.)

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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Date/TimeThumbnailDimensionsUserComment
current21:10, 27 July 2010Thumbnail for version as of 21:10, 27 July 20102,400 × 1,800 (2.92 MB)Smallman12q (talk | contribs)Higher resolution.
21:05, 27 July 2010Thumbnail for version as of 21:05, 27 July 20102,400 × 1,800 (1.25 MB)Sodmy (talk | contribs){{Information |Description={{en|1=This illustration shows one possible mechanism for how the star HE 0437-5439 acquired enough energy to be ejected from our Milky Way galaxy.}} {{uk|1=Еволюція потрійної зоряної системи HE 04

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