Примери за използване на Stellar winds на Английски и техните преводи на Български
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The ions may have been dispersed by stellar winds.
The stellar winds from main sequence stars do not affect the evolution of stars with lower mass.
Different types of stars have different types of stellar winds.
Stellar winds from main-sequence stars do not strongly influence the evolution of lower mass stars such as the Sun.
Away from the viewer,the video also shows the collisions of fast stellar winds creating X-rays.
Stellar winds, pushed away from a massive star's surface by its intense light, can have a profound influence on their environment.
Farther away from the viewer,the movie also shows collisions of fast stellar winds producing X-rays.
When the stellar winds hit dense walls of gas, they create shocks, which generate a new wave of star birth along the wall of the cavity.
Nearby worlds of ice evaporate and form long,comet-like tails driven back by the stellar winds.
This makes it an excellent system for studying the impact of the stellar winds on the parent cloud from which the young star is formed".
The single water jet represents the constant flow of dust particles being created by the colliding stellar winds.
The cloud of glowing gas is over 100 light-years across, sculpted by stellar winds and radiation from embedded open star cluster NGC 1893.
It appears that stellar winds and thermal pulsations produced by 391 Pegasi pulled atmospheric material from the outer layers of the exoplanet and hurled it into space.
This simulation shows how bubbles form over the course of 4.7 million years from the intense stellar winds off a massive star.
It is possible that the radiation and stellar winds from massive stars actually help create denser spots within the pillars, which can then form stars.
Within the nebula, several pillars of dark, dense gas are being shaped by the energetic light and strong stellar winds from the brilliant cluster of thousands of stars.
In addition, Kappa Ceti's stellar winds are 50 times more powerful than our sun's solar wind, ripping through nearby space like a relentless plasma hurricane.
A gas giant can't form that close to their star, because the gravity, radiation,and intense stellar winds ought to keep the gas from clumping together.
Massive stars of types O and B have stellar winds with lower mass loss rates( M˙< 10- 6{\displaystyle\scriptstyle{\dot{M}} 1- 2000 km/s).
We thought that very massive stars with the chemical composition typical of our galaxy must shed most of their gas in powerful stellar winds, as they approach the end of their life".
Over time, stellar winds and supernovae deposit the metals into the surrounding environment, enriching the interstellar medium and providing recycling materials for the birth of new stars.
The"wings" of the nebula are actually bubbles of hot gas created by stellar winds and high energy radiation coming from a massive, hot, newborn star in the center.
The heliopause is the theoretical boundary where the Sun's solar wind is stopped by the interstellar medium;where the solar wind's strength is no longer great enough to push back the stellar winds of the surrounding stars.
Other astronomers believe fluorine may come from supernova explosions or stellar winds, but the new study suggests that red giants are the main suppliers.
Hubble reveals an important population of stars with strong stellar winds, signified by excess emission from ionized gas at one infrared wavelength(1.87 microns) compared to another slightly different wavelength(1.90 microns).
This issue was generally resolved in the late 1990s when new computer simulations,which included the effects of mass loss due to stellar winds, indicated a much younger age for globular clusters.
The wild discrepancy between the speed of Apep's rapid stellar winds and that of the unhurried dust pinwheel is thought to result from one of the stars in the binary launching both a fast and a slow wind- in different directions.
From the vantage point of the Milky Way's supermassive black hole, Sgr A*, the viewer can see about 25 Wolf-Rayet stars(white, twinkling objects)as they continuously eject stellar winds(black to red to yellow color scale).
It plays an equally important role in the formation of galaxies,the solar and stellar winds, and what may become one of the biggest societal applications of plasma physics: controlled fusion energy.
The chemical composition of our galaxy's most massive stars suggests that they lose most of their mass at the end of their lives through explosions and powerful stellar winds, before the star's core collapses into a black hole.