Resolving a shocked high-velocity cloud in the Leading Arm

Details Resolving a shocked high-velocity cloud in the Leading Arm Resolving a shocked high-velocity cloud in the Leading Arm

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atnf.prop.2555m&link_type=abstract

ATNF proposal C1675, Semester: October, 2009

Mathematics

Logic

Interstellar Medium In And Around The Milky Way, Magellanic Clouds, Atca

Scientific paper

Galaxies' ecology and evolution are driven by recycling and accretion of gas within the interstellar medium. These in turn are governed by poorly-understood physical processes acting on small scales. By observing in one particular sightline, toward omega Centauri, we can study several key features of these processes: (1) accretion of gas onto the Galactic Disc, by observing a disrupted high-velocity cloud; (2) small-scale chemical, kinematic and morphological structures in the foreground ISM, through comparison with other tracers such as dust emission and atomic and molecular optical line absorption; (3) the unexplained removal of gas from globular clusters, by observing omega Centauri itself.

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