Rapid disappearance of a warm, dusty circumstellar disk

Carl Melis (), B. Zuckerman, Joseph H. Rhee, Inseok Song, Simon J. Murphy and Michael S. Bessell
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Carl Melis: Center for Astrophysics and Space Sciences, University of California
B. Zuckerman: University of California
Joseph H. Rhee: California State Polytechnic University, Pomona, Pomona, California 91768, USA
Inseok Song: University of Georgia
Simon J. Murphy: Research School of Astronomy and Astrophysics, College of Mathematical and Physical Sciences, The Australian National University, Cotter Road, Weston Creek, Australian Capital Territory 2611, Australia
Michael S. Bessell: Research School of Astronomy and Astrophysics, College of Mathematical and Physical Sciences, The Australian National University, Cotter Road, Weston Creek, Australian Capital Territory 2611, Australia

Nature, 2012, vol. 487, issue 7405, 74-76

Abstract: Observations of a young, Sun-like star indicate that orbiting debris from the process of terrestrial planet formation has undergone an unprecedented phase of rapid evolution that cannot be explained by any known physical model.

Date: 2012
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DOI: 10.1038/nature11210

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