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Dynamical Mass Ratios of the Youngest Low-Mass Stars

Dynamical Mass Ratios of the Youngest Low-Mass Stars. Gregory Mace Mentor: Lisa Prato Northern Arizona University Physics and Astronomy. This Project. Goal: To measure mass ratios of very young binary stars. Why: To calibrate the parameters used in models of young star formation.

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91 spt k7 m0 - PowerPoint PPT Presentation

Dynamical Mass Ratios of the Youngest Low-Mass Stars