The Newly Discovered Nova Super-remnant Surrounding Recurrent Nova T Coronae Borealis: Will it Light Up during the Coming Eruption?

A century or less separates the thermonuclear-powered eruptions of recurrent novae (RNe) in the hydrogen-rich envelopes of massive white dwarfs. The colliding ejecta of successive RN events are predicted to always generate very large (tens of parsecs) super-remnants; only two examples are currently...

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Principais autores:	Michael M. Shara, Kenneth M. Lanzetta, Alexandra Masegian, James T. Garland, Stefan Gromoll, Joanna Mikolajewska, Mikita Misiura, David Valls-Gabaud, Frederick M. Walter, John K. Webb
格式:	Artigo
語言:	Inglês
出版:	IOP Publishing 2024-01-01
叢編:	The Astrophysical Journal Letters
主題:	Novae Recurrent novae
在線閱讀:	https://doi.org/10.3847/2041-8213/ad991e
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