Examples of using Main sequence star in English and their translations into Vietnamese
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Ecclesiastic
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Computer
including a subgiant or(if the orbit is sufficiently close) even a main sequence star.
M37 has at least a dozen red giants and its hottest surviving main sequence star is of stellar classification B9 V. The abundance of elements other than hydrogen
The spectrum of V838 Monocerotis reveals a companion, a hot blue B-type main sequence star probably not very different from the progenitor star,[15] it is also possible that the progenitor was slightly less massive than the companion
termed Sirius A, is a main sequence star of spectral type A1V,
The visible component is an F-type main sequence star with a stellar classification of F6 V.[2] It is around 2.4 billion years old[3]
and is about 1.4 times its radius.[7] It has a stellar classification of A3 V,[3] which means it is an A-type main sequence star that is generating energy at its core through the nuclear fusion of hydrogen.
classification of A3 Va,[3] with the luminosity class'Va' indicating this is a particularly luminous dwarf, a main sequence star that is generating energy through the nuclear fusion of hydrogen at its core.
The primary member of this system is a massive, B-type main sequence star with a stellar classification of B6 V. It is a close spectroscopic binary with an orbital period of 3.854 days, an eccentricity of 0.04, and a combined visual magnitude of 5.30.
which indicates this is a B-type main sequence star. Its total luminosity is 3300[12] times that of the Sun while it has a surface temperature of 18,890 K.[8]
This is an A-type main sequence star with a stellar classification of A1 V.[3] It has a high rate of
Gamma Serpentis is an ordinary F-type main sequence star with a stellar classification of F6 V.[1] It is larger
indicates that this is a main sequence star with enhanced levels of strontium(Sr), chromium, and europium(Eu)
Most main sequence stars are dwarf stars. .
The AD Andromedae system consists of two close main sequence stars of spectral type A0V.
Be stars are primarily considered to be main sequence stars, but a number of subgiants
Of the main sequence stars in the cluster, 79%±1% are from the first generation
Blue and white supergiants are high luminosity stars somewhat cooler than the most luminous main sequence stars.
Several decades of SETI analysis have not revealed any main sequence stars with unusually bright or meaningfully repetitive radio emissions, although there have been several candidate signals.
therefore all red dwarfs are main sequence stars.
composed of two K class(orange) main sequence stars, the brighter 61 Cygni A