Massive clouds of gas,
discovered long ago but only recently identified as being within the margins of
the Milky Way, play a key role in the ability of the galaxy to churn out new stars
by raining gas onto the plane of the galaxy, a new report suggests. Writing
this week in the scientific journal Nature, Bart P. Wakker, a University of
Wisconsin-Madison astronomer, and colleagues have chipped away at a
three-decade-old mystery about the nature and role of what astronomers call
high-velocity clouds. In the process, they've discovered a mechanism by which
the galaxy is seeded with the stuff of stars and solved a long-standing
question of galactic evolution.
Photo Credits: Image
composite by Ingrid Kallick of Possible Designs, Madison Wisconsin. The
background Milky Way image is a drawing made at Lund Observatory. High-velocity
clouds are from the survey done at Dwingeloo Observatory (Hulsbosch &
Wakker, 1988).