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Examples ofspectroscopic binary
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This is aspectroscopicbinarywith an angular separation of 0.2 arcseconds between the two components.
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This example is from Wikipedia and may be reused under a CC BY-SA license.In the past it was suggested that it may be aspectroscopicbinary.
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This example is from Wikipedia and may be reused under a CC BY-SA license.This is aspectroscopicbinarystar system with an estimated period of 2,500 days.
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This example is from Wikipedia and may be reused under a CC BY-SA license.In the past, this star catalogued as aspectroscopicbinaryand a companion was apparently detected through lunar occultation.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.It is aspectroscopicbinarywhose two components are separated by 0.1 arcseconds.
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This example is from Wikipedia and may be reused under a CC BY-SA license.The system is both a visual andspectroscopicbinary.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.Conversely,spectroscopicbinarystars move fast in their orbits because they are close together, usually too close to be detected as visual binaries.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.The primary is also aspectroscopicbinary, and has an unresolved companion, meaning the system has at least four components.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.It is aspectroscopicbinary, and it has an unresolved companion which has an orbital period of 389 days.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.The brightest component is aspectroscopicbinarywith an orbital period of 56.71 days and an eccentricity of 0.17.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.Aspectroscopicbinaryis called double-lined when the absorption lines of both stars can be observed with a spectroscope.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.It is also aspectroscopicbinarywith an orbital period of 0.262 days.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.In 1898 this system was reported to be aspectroscopicbinarysystem, with an orbital period of 280.55 days.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.It was recognized as aspectroscopicbinarystar in 1922, and its orbital solution published in 1984; it has a 596-day orbital period.
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This example is from Wikipedia and may be reused under a CC BY-SA license.It became important because the effect called into question the values of parameters such as mass and luminosity ratios in massivespectroscopicbinarysystems.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.The inner components form aspectroscopicbinarywith a period of 6.1 years (2,238.7 days) and an orbital eccentricity of 0.3530.
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This example is from Wikipedia and may be reused under a CC BY-SA license.The inner pair is aspectroscopicbinarythat completes an orbit with a period of 72 days.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.This is aspectroscopicbinarysystem with an orbital period of 0.6 days.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.The inner pair of stars in this system form aspectroscopicbinarywith a combined magnitude of 5.44 and an orbital period of 1.302 days.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.It is aspectroscopicbinary, whose components are separated by 0.176 arcseconds.
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Wikipedia
This example is from Wikipedia and may be reused under a CC BY-SA license.These examples are from corpora and from sources on the web. Any opinions in the examples do not represent the opinion of the Cambridge Dictionary editors or of Cambridge University Press or its licensors.