[permalink] [id link]
Beta Canis Minoris shows little variation in brightness, but it does display changes in the hydrogen emission coming from the gaseous disk.
from
Wikipedia
Some Related Sentences
Beta and Canis
Beta Cephei ( β Cep ) variables, or Beta Canis Majoris variables, as these stars are sometimes called, especially in Europe ) undergo short period pulsations in the order of 0. 1 – 0. 6 days with an amplitude of 0. 01 – 0. 3 magnitudes ( 1 % to 30 % change in luminosity ).
The primary is a variable star considered to be the prototype of its subclass of pulsating variable stars, which are sometimes named for Beta Canis Majoris.
Beta Canis Minoris ( β CMi, β Canis Minoris ) is a star in the constellation of Canis Minor.
Beta Canis Minoris has about 3. 5 times the Sun's mass and is rotating rapidly with a projected rotational velocity of, which gives a lower bound on the azimuthal rotational velocity along the star's equator.
Canis Minoris, Beta
fr: Beta Canis Minoris
id: Beta Canis Minoris
pt: Beta Canis Minoris
Artist's conception of the Local Bubble ( containing the Sun and Beta Canis Majoris ) and the Loop I Bubble ( containing Antares ).
Other stars in this association include Alpha Pictoris, Beta Canis Minoris and the open cluster IC 2391.
Beta Canis Majoris ( β CMa, β Canis Majoris ) is a star in the southern constellation of Canis Major, the ' greater dog ', and is located at a distance of about 500 light-years ( 150 parsecs ) from the Earth.
In any case, the name was somehow applied to both Delta Canis Majoris and Beta Columbae.
( At the time he actually identified is as a Beta Canis Majoris star, which was subsequently designated a Beta Cephei variable.
# redirect Beta Canis Majoris
# redirect Beta Canis Minoris
# redirect Beta Canis Majoris
# redirect Beta Canis Majoris
Beta and Minoris
Beta Ursae Minoris ( β UMi, β Ursae Minoris ) is the brightest star in the bowl of the " Little Dipper " ( which is part of the constellation Ursa Minor ), and only slightly fainter than Polaris, the northern pole star and brightest star in Ursa Minor.
Ursae Minoris, Beta
eu: Beta Ursae Minoris
fr: Beta Ursae Minoris
fi: Beta Ursae Minoris
* Dubhe and Merak ( Alpha and Beta Ursae Majoris ), the two stars at the end of the bowl of the Big Dipper are habitually called The Pointers: a line from β to α and continued for a bit over five times the distance between them, arrives at the North Celestial Pole and the star Polaris ( α UMi / Alpha Ursae Minoris ), the North Star.
This meteor shower is named for its radiant point which is located near the star Beta Ursae Minoris ( Kochab ) in the constellation Ursa Minor.
# redirect Beta Ursae Minoris
Together with Beta Ursae Minoris, or Kochab, Gamma forms the end of the dipper pan of the " Little Dipper ", which is a colloquial name for the constellation.
# redirect Beta Ursae Minoris
Beta and shows
* The ending scene shows the Enterprise approaching colony Beta VI, an Earthlike planet.
Phi Beta has completed several national projects including: hand enlarging music for the visually impaired, service in USO shows, aid to music programs in Mexico, and most notably her continued work with the MacDowell Colony.
The prototype of these variable stars, Beta Cephei, shows variation in apparent magnitude from + 3. 16 to + 3. 27 with a period of 4. 57 hours.
Beta and little
They find the inhabitants of Beta III ( who seem to be modeled after 19th-century Earth ) are a very static culture, with little or no individual expression or creativity.
Thus book 1 is called Alpha ( Α ); 2, little alpha ( α ); 3, Beta ( Β ); 4, Gamma ( Γ ); 5, Delta ( Δ ); 6, Epsilon ( Ε ); 7, Zeta ( Ζ ); 8, Eta ( Η ); 9, Theta ( Θ ); 10, Iota ( Ι ); 11, Kappa ( Κ ); 12, Lambda ( Λ ); 13, Mu ( Μ ); 14, Nu ( Ν ).
Beta and variation
It is a Beta Cephei-type Cepheid variable with a variation of less than 0. 1 magnitudes.
Along with Delta Cephei, Zeta Geminorum and Beta Doradus, it is one of the most prominent naked eye Cepheids ; that is, both the star itself and the variation in its brightness can be distinguished with the naked eye.
In addition to brightness variation due to eclipses, the system is also an RS Canum Venaticorum type or Beta Lyrae type variable star.
Beta and brightness
Beta Pegasi is a semi-regular variable with a period of 43. 3 days and a brightness that varies from magnitude + 2. 31 to + 2. 74.
Delta Crucis is a strong candidate Beta Cephei variable and changes its brightness subtly with a period of 1. 3 hours.
Beta Cephei variables are variable stars which exhibit variations in their brightness due to pulsations of the stars ' surfaces.
Typically, Beta Cephei variables change in brightness by 0. 01 to 0. 3 magnitudes with periods of 0. 1 to 0. 6 days.
It is classified as a Beta Cephei type variable star and its brightness varies by 0. 01 magnitudes.
Beta and does
) And though Reed does not award Latin honors to graduates, Reed does confer several awards for academic achievement at the time of commencement, including naming students to Phi Beta Kappa.
As of 2010, the Windows version, often referred to informally as " WinScore ", does exist in a Beta version, and is being used by a number of the more proficient and experienced customers.
" Beta version ( 4. 99. xx ), of course, can be tested for free, because in this stadium of development it does not yet represent a complete program.
That is, " How does the bond shared between Phi Beta Sigma and Zeta Phi Beta stands out from any the bonds that are claimed by other Black Greek Lettered Organizations?
Beta does not nest in gamma, quantified modal logic being more than even Peirce could envisage.
Beta decay of fission products of mass 95-98 stops at the stable isotopes of molybdenum of those masses and does not reach technetium.
Beta emissions are also severely attenuated by air ; their range generally does not exceed and intensity rapidly diminishes with distance.
He is the only founder of Beta Theta Pi for which a photo does not exist ( or yet to be found ).
0.696 seconds.