Credit & Copyright: X-ray -
NASA,CXC,SAO,
R. Montez et al.;
Optical -
Adam Block,
Mt. Lemmon SkyCenter,
U. Arizona
Explanation:
A long recognized naked-eye
variable star, R Aquarii
is actually an interacting binary star system, two
stars that seem to have a
close,
symbiotic relationship.
About 710 light years away, it consists of a cool red giant star
and hot, dense white dwarf star in mutual orbit around their common
center of mass.
The binary system's visible light is dominated by the red giant,
itself a Mira-type long period variable star.
But material in cool giant star's extended envelope is pulled by gravity
onto the surface of the smaller, denser white dwarf,
eventually triggering
a thermonuclear explosion and blasting material into space.
Optical image data (red) shows the still expanding ring of debris
originating from a blast that would have been seen in the early 1770s.
The
evolution of less understood energetic events producing
high energy emission in the R Aquarii system has been
monitored since 2000 using Chandra X-ray Observatory data (blue).
The composite field of view is less that a light-year across at the
estimated distance of R Aquarii.
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Publikacii s klyuchevymi slovami:
symbiotic star - simbioticheskie sistemy
Publikacii so slovami: symbiotic star - simbioticheskie sistemy | |
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Sm. takzhe:
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