Linford, Justin D.Chomiuk, LauraSokoloski, Jennifer L.Weston, Jennifer H. S.Horst, Alexander J. van derMukai, KojiBarrett, PaulMioduszewski, Amy J.Rupen, Michael2019-12-172019-12-172019-10-07Linford, Justin D.; Chomiuk, Laura; Sokoloski, Jennifer L.; Weston, Jennifer H. S.; Horst, Alexander J. van der; Mukai, Koji; Barrett, Paul; Mioduszewski, Amy J.; Rupen, Michael; T CrB: Radio Observations during the 2016–2017 "Super-active" State; The Astrophysical Journal 884,1 (2019); https://iopscience.iop.org/article/10.3847/1538-4357/ab3c62https://doi.org/10.3847/1538-4357/ab3c62http://hdl.handle.net/11603/16756We obtained radio observations of the symbiotic binary and known recurrent nova T Coronae Borealis following a period of increased activity in the optical and X-ray bands. A comparison of our observations with those made prior to 2015 indicates that the system is in a state of higher emission in the radio as well. The spectral energy distributions are consistent with optically thick thermal bremsstrahlung emission from a photoionized source. Our observations indicate that the system was in a state of increased ionization in the companion wind, possibly driven by an increase in accretion rate, with the radio photosphere located well outside the binary system.8 pagesen-USThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.©2019. The American Astronomical Society. All rights reserved.binariessymbioticnovaecataclysmic variablesradio continuumstarsindividual (T CrB)white dwarfsText