Examples of 'sequence stars' in a sentence
Meaning of "sequence stars"
sequence stars: To identify, arrange, or classify stars based on their order or properties within a series
How to use "sequence stars" in a sentence
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sequence stars
Both companions are white main sequence stars.
O class main sequence stars are already highly luminous.
This band is called the main sequence stars.
The components are main sequence stars of similar size and appearance.
These are the rarest of all main sequence stars.
Main sequence stars derive energy from the fusion of hydrogen into helium in their cores.
Astronomers call such stars main sequence stars.
Which element do main sequence stars primarily use for nuclear fusion?
The two components are yellow main sequence stars.
Located above the main sequence stars in the H-R diagram.
This means that hot supergiants lie on a relatively narrow band above bright main sequence stars.
White main sequence stars.
Eventually they become optically visible on the stellar birthline as pre-main sequence stars.
It is composed of two white main sequence stars in close orbit.
The Main Sequence Stars as per the Morgan-Keenan spectral classification.
See also
Not all stars will become main sequence stars.
The earliest main sequence stars are of type A0.
Luminosity class V includes all main sequence stars.
The brightest main sequence stars are of spectral type B7.
Both stars are F-type main sequence stars.
The brightest main sequence stars are of sprectral type B7.
Both components are rapidly rotating A-type main sequence stars.
Both component stars are detached main sequence stars which do not fill their Roche lobes.
The inner components of this system consist of a pair of B-type main sequence stars.
Completing the triangle are the two white main sequence stars Beta and Gamma Trianguli Australis.
On the opposite end of the spectrum, are the large blue, main sequence stars.
It consists of two B-type main sequence stars that orbit each other.
The stars are usually A0 to F5 type giant or main sequence stars.
Therefore, the hotter main sequence stars are, the brighter they are.
A red giant is a star lacking a photosphere, the “ surface ” from which main sequence stars emit radiation.
The components are main sequence stars of spectral types B9V and A3V.
Herbig Ae / Be stars are pre-main sequence stars.
Both are A-type main sequence stars with a stellar classification of A2 Vs.
All supergiants are larger and more luminous than main sequence stars of the same temperature.
It consists of two main sequence stars that orbit each other every 9.86 days.
BI 253 is one of the hottest, most massive, and most luminous known main sequence stars.
These stars are chemically peculiar main sequence stars of spectral class B8p to A7p.
The AD Andromedae system consists of two close main sequence stars of spectral type A0V.
All seem to be near equally hot B class main sequence stars that weigh between 3 to 4 M ☉.
The two eclipsing stars are almost identical class B main sequence stars with masses around 18 M ☉.
There are seven types of main sequence stars in the galaxy, [ 2 ].
Westerlund 2 also contains a large number of pre-main sequence stars with masses below 2.5 M ☉.
Gliese 667 is a triple star system with two K-type main sequence stars and a red dwarf.
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