「coronae」の共起表現(1語右で並び替え) - Weblio英語共起表現検索


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「coronae」の共起表現一覧(1語右で並び替え)

該当件数 : 32



Coronae appear on both the planet Venus and Uranus's
On Venus, coronae are large (typically several hundred kilometr
Coronae are thought to form due to the upwelling of h
It is believed that coronae are formed when plumes of rising hot material
Beta Coronae Australis (Beta CrA, β Coronae Australis, β C
Both V691 Coronae Australis and 2MASS J18242041-3715138 are wit
An X-ray source is in orbit around V691 Coronae Australis, which is of unknown spectral type.
Variable star R Coronae Borealis type.
Alpha Coronae Borealis (α CrB, α Coronae Borealis) is a bin
Beta Coronae Borealis (Beta CrB, β Coronae Borealis, β CrB
DY Persei variables are a subclass of R Coronae Borealis variables.
S Coronae Borealis (S CrB) is a Mira-type long period v
T Coronae Borealis (T CrB), informally nicknamed the Bl
Kappa Coronae Borealis b is an extrasolar planet approximat
R Coronae Borealis is a yellow supergiant star, and is
R Coronae Borealis itself normally shines at approximat
la Abell 58, exhibiting features similar to R Coronae Borealis variable stars (RCBs), but also pecu
It belongs to the very rare R Coronae Borealis class of variables which are often c
Kappa Coronae Borealis is a star approximately 102 light ye
a small variation in the radial velocity of β Coronae Borealis with a periodicity of 320 days, sugg
AAVSO light curve showing R Coronae Borealis' behavior over approximately 8 years
The B, G and R components of 73P, and Tau Coronae Borealis, May 1, 2006.
rs such as Sirius itself, Beta Aurigae, Alpha Coronae Borealis, Zeta Crateris, and Beta Serpentis.
208 days or 3.307 years to orbit around Kappa Coronae Borealis.
Study of the Proposed Planetary System of Rho Coronae Borealis”, Ap J 548, L61.
r of the Crown of Thorns (Festum susceptionis coronae Domini) was instituted at Paris in 1239, when
In planetary geology, a corona (plural: coronae) is an oval-shaped feature.
The two coronae may have formed at the same time over a singl
Lower than solar Fe abundance in the coronae of active stars
See also: List of coronae on Venus
Aphnaeus coronae Talbot, 1935
Coronae were first identified in 1983, when the radar
                                                                                                   


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