pre-main-sequence star oor Slowaaks
pre-main-sequence star
Vertalings in die woordeboek Engels - Slowaaks
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en
star in the stage when it has not yet reached the main sequence
Geskatte vertalings
Vertoon algoritmies gegenereerde vertalings
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These pre-main-sequence stars are often surrounded by a protoplanetary disk and powered mainly by the conversion of gravitational energy.
Pre núdzové prípady je vhodné mať v zásobe primerané množstvo kolostraWikiMatrix WikiMatrix
A pre-main-sequence star (also known as a PMS star and PMS object) is a star in the stage when it has not yet reached the main sequence.
Meteorologické podmienkyWikiMatrix WikiMatrix
The astronomer Louis G. Henyey and his colleagues in the 1950s, showed that the pre-main-sequence star can remain in radiative equilibrium throughout some period of its contraction to the main sequence.
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Pre-main-sequence stars become optically visible after stellar birthline.
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When the surrounding gas/dust envelope disperses and accretion process stops, the star is considered as pre-main-sequence star.
Európske spoločenstvo a Spojené štáty americké sa domnievajú, že normy pripojené k tejto dohode poskytujú takýto spoločný rámec a základ pre spoluprácu v oblasti ďalšieho vývoja a implementácie noriem svojimi príslušnými kompetentnými orgánmiParaCrawl Corpus ParaCrawl Corpus
On the Hertzsprung–Russell diagram, the pre-main-sequence stage of stars with masses less than 0.5 solar masses translates into a move along Hayashi tracks (almost vertically down) and later along Henyey tracks (almost horizontally to the left, towards the main sequence).
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Location of the target stars in the HR diagram together with the Pre-Main Sequence evolutionary tracks (solid curves) and isochrones (dotted curves) based on the Pisa Stellar Models (Tognelli et al.
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7 sinne gevind in 14 ms. Hulle kom uit baie bronne en word nie nagegaan nie.