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A Multiwavelength View of $ρ$ Oph II: Disentangling the Variability of the Multi-Star Component C
We present a multiwavelength analysis of the star $ρ$ Oph C, covering X-ray, optical, near-infrared, and radio observations to test for the presence of interferometrically-detected cool star companions. The X-ray observations from Chandra, XMM-Newton, and NuSTAR show flare-like events lasting minute
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