Exemples d'utilisation de Binary star en Anglais et leurs traductions en Français
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η Sagittarii, η Sgr) is a binary star system in the southern zodiac constellation of Sagittarius.
Centauri Mizar is often said to have been the first binary star discovered when it was observed in 1650 by Giovanni Battista Riccioli,
Separated from its brighter companion by 108 arcseconds in the sky is the binary star μ2 Boötis, which has a combined spectral type of G1V and a combined brightness of +6.51 magnitudes.
It has an overall apparent visual magnitude of approximately 5.15 and is a spectroscopic binary star which consists of two giant stars,
It is a binary star with a blue-white main sequence star companion likely to be of spectral type B3V to B5V with a mass of just over five solar masses, one of the hottest
They are not a binary star, in that they are not gravitationally linked, but they are close
is known to be a binary star system.
the Algol paradox is a paradoxical situation when elements of a binary star seem to evolve in discord with the established theories of stellar evolution.
temperature changes was largely dismissed in favour of orbital motions of a binary star.
I take it my calculations help explain the"protabations" you have been seeing… in the rotation pattern of your binary star, but have been unable to explain until… this moment.
An eclipsing binary star is a binary star system in which the orbit plane of the two stars lies so nearly in the line of sight of the observer that the components undergo mutual eclipses.
A thermonuclear supernova is the explosion of a white dwarf in a binary star system, triggered by thermonuclear reactions in matter from a companion star accreted on the surface of the white dwarf.
It is a spectroscopic binary star and rotating ellipsoidal variable;
conflicted with currently accepted models of tidal movements derived from observations of the orbits of binary star systems.
around 1 degree southeast of the eclipsing binary star U Coronae Borealis.
The most likely scenario that could have created these runaway stars is a collision between two binary star systems, with the stars being ejected along different trajectories radial to the point of intersection.
which would make WOH G64 a binary star although there has been no confirmation of this observation and the intervening dust
class of stellar objects, and Kepler-16b, a well-characterized planet orbiting a binary star.
The fact that the pre-merger black holes were present in a binary star system, as well as the fact that the system was compact enough to merge within the age of the universe, constrains either binary star evolution or dynamical formation scenarios,
One scenario involves an AM CVn type of symbiotic binary star composed of two helium-core white dwarfs surrounded by a circumbinary helium accretion disk formed during mass transfer from the less massive to the more massive white dwarf.