Gas in Debris Disks

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We consider current observations of gas within debris disks systems such
as β Pic. While there is clearly some gas present, the evidence
for molecular hydrogen is, at best, weak. It is possible that these
systems have more mass in dust than in gas -- very different from the
interstellar dark clouds from which stars form, but similar to comets.

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