Type of stellar remnant composed mostly of electron-degenerate matter.
португальский
anã branca 1
Pushing a white dwarf into the solar system, to carry it away.
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The gravity of the white dwarf attracts the red giant's ejected material.
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The more massive the white dwarf is, the slower the pulses get.
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Nothing bright remains save a scattering of dim red and white dwarf stars.
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They can slowly burn down to the level of a white dwarf star.
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When you dump matter on a white dwarf, it undergoes tidal compression heating.
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Hubble also measured the brightness of exploding white dwarf stars -Type 1A supernovas.
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The smaller, denser white dwarf seems to be sucking material off its larger companion.
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Its parent stars are a small, dense white dwarf star and a quickly rotating pulsar.
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The star we're heading for is a white dwarf.
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A white dwarf star, bright but unwelcoming to life.
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In other words, it leaves a white dwarf.
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They couldn't see a white dwarf from here.
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A white dwarf star, Padronis had no companions in space, no planets or asteroids in orbit.
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That damned white dwarf was close enough now to show a tiny disk, swiftly growing larger.
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They had checked the time required for them to see that the white dwarf had gone out.
