T CrB: Radio Observations during the 2016-2017 "Super-active" State

We 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...

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Veröffentlicht in:	The Astrophysical journal 2019-10, Vol.884 (1), p.8
Hauptverfasser:	Linford, Justin D., Chomiuk, Laura, Sokoloski, Jennifer L., Weston, Jennifer H. S., van der Horst, Alexander J., Mukai, Koji, Barrett, Paul, Mioduszewski, Amy J., Rupen, Michael
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics binaries: symbiotic Bremsstrahlung Companion stars Deposition Emission Ionization novae, cataclysmic variables Photoionization Photosphere Radio radio continuum: stars Radio observation stars: individual (T CrB) Stellar winds white dwarfs
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