The wealth of information in this Hubble survey, including seeing stars of all sizes in one dense place, provides an extraordinary opportunity to study star formation. Our goal is to calculate the masses and ages for these young stars so that we can map their history and get a general census of the star formation in that region. We can then sort the stars by mass and age and look for trends.
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Our goal is to calculate the masses and ages for these young stars, so that we can map their history and get a general scenario of the star formation in that region.
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