Examples of using Binary system in English and their translations into Swedish
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Colloquial
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Official
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Medicine
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Ecclesiastic
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Ecclesiastic
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Official/political
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Computer
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Programming
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Political
The unusual star is part of a binary system with a red dwarf,
would continue with the final velocity it possessed when it was a member of a close orbiting binary system.
The latter pair form a binary system located at an angular separation of 52 arcseconds from the primary.
is part of a binary system with a red dwarf.
a white dwarf in a binary system[2].
The reality is that only a small fraction of black holes is in binary system, but so far it's the only way to detect them.
Typically a barium star belongs to a binary system and the anomalies in abundances are explained by mass transfer from a companion white dwarf star.
is part of a binary system.
Another possible mechanism for producing luminosity variations in a star is to have the star itself move in a binary system.
The binary system as a whole has some similarities to the nearby system of Sirius,
This pair may form an eclipsing binary system with a period of 785 days(2.15 years),
We know, because it is located in a binary system with a star in palmacci the Sun.
The binary system as a whole has some similarities to the nearby system of Sirius,
Alternative scenarios require either the evolution of a triple star system, or a binary system with highly eccentric orbit resulting in grazing interactions.
Most Am stars form part of a binary system in which the rotation of the stars has been slowed by tidal braking.
Both components of the binary system are white A-type main sequence stars
One of the most famous red giants in the sky is called Mira A, part of the binary system Mira which lies about 400 light-years from Earth.
They suggested that the magnetar formed through the interactions of two very massive stars orbiting one another in a binary system so compact that it would fit within the orbit of the Earth around the Sun.
The inner pair is a visual binary system consisting of two A-type main-sequence stars with an orbital period of 23.2 years(8,487.9 d),
for example the second star in a binary system, forming an accretion disc.