CIRCUMBINARY RING, CIRCUMSTELLAR DISKS, AND ACCRETION IN THE BINARY SYSTEM UY AURIGAE
Recent exo-planetary surveys reveal that planets can orbit and survive around binary stars. This suggests that some fraction of young binary systems which possess massive circumbinary (CB) disks may be in the midst of planet formation. However, there are very few CB disks detected. The streaming gas...
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Veröffentlicht in: | The Astrophysical journal 2014-09, Vol.793 (1), p.1-14 |
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Sprache: | eng |
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