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词汇 protostar
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Examples of protostar


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The small dark areas in the photograph are believed to be protostars.
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When the protostellar cloud has approximately reached the stable condition of hydrostatic equilibrium, a protostar forms at the core.
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The protostar, at first, only has about 1% of its final mass.
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Adopting larger ages allows protostars to radiate the same amount of energy over a longer time, reducing their average luminosity.
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Over the course of millions of years, these protostars settle down into a state of equilibrium, becoming what is known as a main-sequence star.
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Infrared can also be used to detect protostars before they begin to emit visible light.
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There is mounting evidence that at least some massive protostars are indeed surrounded by accretion disks.
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It is associated with a massive (10 solar masses) protostar, which accretes gas from a disk that surrounds it.
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When destabilized, cloud fragments can collapse under the influence of gravity, to form a protostar.
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If, however, the mass of the protostar is less than about 0.08 solar mass, normal hydrogen thermonuclear fusion reactions will not ignite in the core.
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Within 50 million years, the pressure and density of hydrogen in the centre of the protostar became great enough for it to begin thermonuclear fusion.
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The protostar is now considered a young star since its mass is fixed, and its future evolution is now set.
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Every eleven years, one of the protostars emits a neutron blast that the pilgrims consider a sacred event.
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This class consists of two groups of objects: protostars and premain sequence stars.
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While the surrounding matter is falling onto the central condensation, it is considered to be a protostar.
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A protostar grows by accretion, acquiring mass from its surrounding envelope of interstellar dust and gas.
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Millimeter-wave emission line studies have also provided evidence for the infall of material onto an accreting protostar.
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The outer envelope then accretes onto the central protostar.
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A protostar may have too little mass to become a star.
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This star formation begins enshrouded in the collapsing cloud, blocking the protostars from sight but allowing infrared observation.
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