Radio flux densities of massive stars in the Arches cluster imply an age of about 2.5 Myr and a top-heavy IMF, with mass near 27,000 solar masses under an infrared prior.
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Constraining young massive cluster properties with radio-continuum observations: The Arches cluster
Radio flux densities of massive stars in the Arches cluster imply an age of about 2.5 Myr and a top-heavy IMF, with mass near 27,000 solar masses under an infrared prior.