interacting binary star oor Spaans
interacting binary star
Vertalings in die woordeboek Engels - Spaans
estrella binaria interactuante
Geskatte vertalings
Vertoon algoritmies gegenereerde vertalings
voorbeelde
Advanced filtering
Voorbeelde moet herlaai word.
However, a modified approach resulted in a new formalism that is considered a significant step forward in efforts to model interacting binary-star systems.
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Most recently he has been studying the polarization produced in cataclysmic variables, or interacting binary star systems that give off sudden bursts of intense energy, and dust about young stars.
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However, the interactions between binary star systems prevents further collapse as the cluster approaches middle age.
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The reasons why this premature mass loss occurs are unclear, but the interaction of stars in a binary star system is thought to be one of the main mechanisms.
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As other stars interact with these tight binaries, they increase the energy at the core, which causes the cluster to re-expand.
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The interaction of stars in the collapsed core region causes tight binary systems to form.
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The researchers speculate that the dim, hydrogen-poor supernova's star may have been a moderately massive star in a binary system; in this scenario, the outer layers would have been lost through interactions between the companion stars.
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In the first part, the author talks about stellar evolution and distances, in the second part about binary non-interactive stars, and in the third part about binary interactive stars.
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These are close interacting binary stars, with the primary component (the more massive one) being a white dwarf, and the secondary component usually being a late-type (K-M) star, that is on, or at least close to, the main-sequence.
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The rhythm between communion with God and service toward others in the apostolic life can also be compared to the interaction of binary stars.
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Binary Interactive Stars: Spanish Language Astronomy Materials Education Center
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Title: Binary Interactive Stars
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More about Binary Interactive Stars.
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Knowing the true proportion of interacting high-mass binary stars is therefore crucial to correctly characterise these faraway galaxies. [3]
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This result gives further evidence of the importance of the evolution and the interaction of binary stars for the understanding of many aspects of astrophysics, including subjects that are apparently unrelated such as the chemical evolution of the Universe.
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“Until now”, explains Aníbal García-Hernández, researcher at the IAC and the second author of the article, “various different types of stars had been prepared as candidates: supermassive stars, rapidly rotating massive stars, massive interacting binaries, and massive AGB stars.
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“This result”, concludes Pablo Rodriguez Gil of the IAC and the University of La Laguna, who is another author of the article “is further evidence of the importance of the evolution and the interaction of binary stars for the understanding of many aspects of astrophysics, including subjects which are apparently unrelated such as the chemical evolution of the universe”.
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It is thought that some of the most massive stars (i.e., supermassive stars, rapidly rotating massive stars, massive interacting binaries, and massive AGB stars) in the first generation produce and destroy the heavy elements in their interiors (“nucleosynthesis”) and by rapid mass loss contaminate the interstellar medium where the second generation of stars then forms with different chemical abundances.
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This result is very important because it is the first time that two different components of gas emitting lines due to the same ion have been distinguished by direct imaging. This result gives further evidence of the importance of the evolution and the interaction of binary stars for the understanding of many aspects of astrophysics, including subjects that are apparently unrelated such as the chemical evolution of the Universe.
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Binary stars are celestial bodies that interact as they orbit each other.
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Instead, it is thought that most of them probably originate when dynamical interactions with other stars cause a binary system to coalesce into one star.
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The research program includes the study of white dwarfs (low-mass stars in their final stages of life) within young planetary nebulae and symbiotic stars, the latter being interacting binary systems where a white dwarf is accreting matter from a cool giant star.
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During the twentieth century, astronomers came to understand that most novae could be explained by the runaway explosive behaviour and interactions between two close stars in a binary system.
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This elusive objects, black holes, can be detected only if they interact with matter from stars very near to them in binary star systems.
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Various candidates which might release sodium and aluminium into the interstellar medium have been proposed: massive AGB stars, very massive rapidly rotating stars (spin stars, supernovae...) or very massive interacting binaries.
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36 sinne gevind in 21 ms. Hulle kom uit baie bronne en word nie nagegaan nie.