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Jessica R. Lu Institute for Astronomy University of Hawaii

Jessica R. Lu Institute for Astronomy University of Hawaii

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Proper motions are a powerful tool <strong>for</strong><br />

identifying cluster members.<br />

Commonly used in globular<br />

clusters.<br />

High spatial resolution<br />

optical capabilities <strong>of</strong> HST.<br />

Massive young clusters<br />

require better astrometric<br />

precision.<br />

Massive young clusters<br />

require infrared astrometry.<br />

Anderson+ 2006

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