Examples of 'is a spectroscopic binary' in a sentence
Meaning of "is a spectroscopic binary"
is a spectroscopic binary: This phrase is a term used in astronomy to describe a system of two stars that are so close together that they cannot be individually observed. Instead, their presence is inferred through the analysis of their combined spectra
How to use "is a spectroscopic binary" in a sentence
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is a spectroscopic binary
At least one of the components is a spectroscopic binary.
It is a spectroscopic binary system.
Analysis of its spectrum reveals that it is a spectroscopic binary.
It is a spectroscopic binary star.
Theta2 Crucis, Latinized from θ2 Crucis, is a spectroscopic binary star in the constellation Crux.
A is a spectroscopic binary.
The primary component, Iota Trianguli Australis A, is a spectroscopic binary with a mean apparent magnitude of +5.28.
Boötis is a spectroscopic binary in the constellation Boötes.
The second component is a spectroscopic binary star system.
It is a spectroscopic binary star, located about 3 ° north of Mu Geminorum.
Pi4 Orionis ( π4 Ori, π4 Orionis ) is a spectroscopic binary star in the constellation Orion.
This is a spectroscopic binary system with a stellar classification of A5V.
Omega Draconis ( ω Dra ) is a spectroscopic binary star in the constellation Draco.
This is a spectroscopic binary system with an orbital period of 0.6 days.
Zeta Trianguli Australis ( ζ TrA ) is a spectroscopic binary in the constellation Triangulum Australe.
See also
It is a spectroscopic binary with an orbital period of 134 days.
The primary member, component A, is a spectroscopic binary whose two components are separated by 0.1 arcseconds.
It is a spectroscopic binary whose components have an orbital period of 4028 days.
Zeta Trianguli Australis is a spectroscopic binary star with an apparent magnitude of 4.90.
It is a spectroscopic binary star with the two components orbiting each other every 10.21 days.
Delta Columbae is a spectroscopic binary yellow giant star in the constellation Columba.
Alpha Delphini A is a spectroscopic binary star which has now been resolved using speckle interferometry.
The inner pair is a spectroscopic binary that completes an orbit with a period of 72 days.
S Monocerotis A is a spectroscopic binary system with an orbital period of 74 years.
Iota Orionis is a spectroscopic binary system, with a variable magnitude of O9III.
KQ Puppis ( KQ Pup ) is a spectroscopic binary variable star in the constellation Puppis.
The primary component is a spectroscopic binary whose components have an orbital period of 10.21 days.
HD 93403 is a spectroscopic binary containing two highly luminous hot blue stars.
HR 1884 is a spectroscopic binary star in the constellation Auriga.
Pegasi (56 Peg) is a spectroscopic binary star in the constellation Pegasus.
Andromedae ( 47 And ) is a spectroscopic binary star in the constellation Andromeda.
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