<p>White dwarf star waves. Image 2 of 3. Computer model of waves on the surface of a white dwarf star, a small, dense star formed at the end of a Sun-like star's life. The arrows show the strength and direction of the wind causing the waves. The largest arrows show winds of up to 2000 kilometres per second. The wind comprises hydrogen drawn to the dwarf from an unseen companion star. Such binary systems are called recurrent novae. Hydrogen builds up on the dwarf's surface, and explodes periodically. Turbulent waves explain why dwarf material is seen in the explosions. This is 0. 035 seconds after the wind started. See images R670/139-141 for a sequence of wave development.</p>
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<p>Create the illusion that your new gallery wrapped canvas art is suspended in space with our premium 1.75” inch deep floating frame. With several available frame finishes to choose from, you’re sure to find the color that best accents your handcrafted art and personal décor.</p>
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Alexandros Alexakis
Science
Astronomy
Space
Stars
