Примеры использования Variable star на Английском языке и их переводы на Русский язык
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γ Phoenicis is a spectroscopic binary and a small amplitude variable star.
Wendel using wedge photometer, and was classified as a M6III variable star in 1924.
was a Turkish-American astronomer who was the director of the American Association of Variable Star Observers(AAVSO) from 1973 to 2004.
κ Sco A, is a variable star of Beta Cephei type.
identified with a faint, heavily reddened variable star lying just outside the error box predicted by Uhuru observations.
In the 1920s, Dalmero Francis Brocchi, an amateur astronomer and chart maker for the American Association of Variable Star Observers(AAVSO), created a map of this object for use in calibrating photometers.
NR Vulpeculae is a red supergiant and irregular variable star in the constellation Vulpecula.
wrote Variable Star, based on an outline and notes for a juvenile novel that Heinlein prepared in 1955.
Current field of research involves CCD observations mainly of a long range of variable star types, as well as active galactic nuclei(AGN)- namely blazars.
one-half year sunspot cycles betray that it was a variable star in its youth.
is a massive multiple and variable star system located in the constellation Monoceros.
Variable star observers can compare its brightness with several 4th-
The hands-on astrophysics material uses the unique variable star database of the American Association of Variable Star Observers AAVSO.
Sigma Canis Majoris was noted as a likely variable star in a list of bright southern stars studied at the Cape Observatory.
It is classified as an irregular variable star and its brightness varies from magnitude +4.63 to +4.70.
Visual variable star observers make an estimate of its brightness by comparing its brightness with nearby stars with a known brightness value.
It is classified as a BY Draconis type variable star and its brightness varies by 0.08 magnitudes.
It is a variable star classified as a slow irregular pulsating supergiant, and varies from an
Since its founding in 1911, the American Association of Variable Star Observers(AAVSO) has coordinated, collected, evaluated, analyzed,
NGC 2363-V1 is a luminous blue variable star in the star-forming region NGC 2363,