「coronae」の共起表現(2語左で並び替え)

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共起表現

「coronae」の共起表現一覧(2語左で並び替え)

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The B, G and R components of 73P, and Tau	Coronae Borealis, May 1, 2006.
An X-ray source is in orbit around V691	Coronae Australis, which is of unknown spectral type.
208 days or 3.307 years to orbit around Kappa	Coronae Borealis.
It was known as Variabilis	Coronae, "Variable of Corona".
rs such as Sirius itself, Beta Aurigae, Alpha	Coronae Borealis, Zeta Crateris, and Beta Serpentis.
It is believed that	coronae are formed when plumes of rising hot material
Both V691	Coronae Australis and 2MASS J18242041-3715138 are wit
and structure and energy balance in cool star	coronae.
In planetary geology, a corona (plural:	coronae) is an oval-shaped feature.
Lower than solar Fe abundance in the	coronae of active stars
s a whole, Artemis is not elevated like other	coronae.
See also: List of	coronae on Venus
DY Persei variables are a subclass of R	Coronae Borealis variables.
Study of the Proposed Planetary System of Rho	Coronae Borealis”, Ap J 548, L61.
a small variation in the radial velocity of β	Coronae Borealis with a periodicity of 320 days, sugg
On Venus,	coronae are large (typically several hundred kilometr
It belongs to the very rare R	Coronae Borealis class of variables which are often c
AAVSO light curve showing R	Coronae Borealis' behavior over approximately 8 years
Variable star R	Coronae Borealis type.
The two	coronae may have formed at the same time over a singl
la Abell 58, exhibiting features similar to R	Coronae Borealis variable stars (RCBs), but also pecu

共起表現

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「coronae」の共起表現一覧(2語左で並び替え)