A Multiwavelength View of $\rho$ Oph II: Disentangling the Variability of the Multi-Star Component C
We present a multiwavelength analysis of the star $\rho$ 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 minutes or days in time...