Voorbeelden van het gebruik van Variable stars in het Engels en hun vertalingen in het Nederlands
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Programming
Cataclysmic variable stars(CV) are stars which irregularly increase in brightness by a large factor,
It was optimized for visible and ultraviolet light observations of variable stars and other astronomical objects varying in brightness.
Cataclysmic variable stars are binary stars that consist of two components;
As a result, variable stars after QZ were numbered according to Nijland's system beginning with V335.
Light curves of more than 3000 variable stars of type RRÂ Lyrae
This work later was extended to the Magellanic Clouds, adding a further 2,000,000 observations of variable stars.
Instead of shining with a steady glow… like most stars… variable stars pulsate… brightening
They form the prototype of a class of variable stars known as BY Draconis variables. .
is a list of variable stars.
Symbiotic novae are slow irregular eruptive variable stars with very slow nova-like outbursts with an amplitude of between 9
The Stars During the Day… 21. Spectral Classes… 22. Variable Stars… 23.
RR Lyrae variables are periodic variable stars, commonly found in globular clusters.
Type II Cepheids are variable stars which pulsate with periods typically between 1 and 50 days.
He proposed naming variable stars in each constellation using a simple numbering system beginning with V1, V2,… and so forth.
A possible explanation for some of the discrepancies When we consider the brightness of pulsating variable stars, found in Hubble's constant. we start to see.
while a student he gained an interest in astronomy-studying variable stars.
A possible explanation for some of the discrepancies When we consider the brightness of pulsating variable stars, we start to see found in Hubble's constant.
She then studied variable stars, making over 1,250,000 observations with her assistants.
When we consider the brightness of pulsating variable stars… we start to see a possible explanation… for some of the discrepancies found in Hubble's constant.
When we consider the brightness of pulsating variable stars, a possible explanation for some of the discrepancies.