An illustration shows the HD 142527 binary star system from data captured by the Atacama Large Millimeter/submillimeter Array. The red body orbiting the center represents the low-mass companion star. Click image for a larger version. Illustration by B. Saxton/NRAO/AUI/NSF
Rice Uni Assistant Professor Andrea Isella presented images of binary system HD 142527 by Atacama Large Millimeter/submillimeter Array (ALMA) radio telescope at the annual meeting of the American Association for the Advancement of Science in Washington, D.C. The system has long been known to harbor a planet-forming corona of dust and gas, but ALMA images are providing more detail than ever and allowing for better analysis of the system’s contents and mechanics.
Isella studies the formation of planetary systems...
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