意味 | 共起表現 |
「coronae」の共起表現一覧(1語右で並び替え)
該当件数 : 32件
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 | |
意味 | 共起表現 |
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