29 octubre 2014
Scientists have detected a streamer of dust and gas flowing from a massive outer disk toward the inner reaches of a binary star system. This never-before-seen feature may be responsible for sustaining a second, smaller disk of planet-forming material that otherwise would have disappeared long ago.
http://feeds.sciencedaily.com/~r/sciencedaily/~3/Cj4iCg6w-zM/141029141221.htm
