Journal ArticleThe Newly Discovered Nova Super-remnant Surrounding Recurrent Nova T Coronae Borealis: Will it Light Up during the Coming Eruption?Shara, Michael M; Lanzetta, Kenneth M; Masegian, Alexandra; Garland, James T; Gromoll, Stefan; Mikolajewska, Joanna; Misiura, Mikita; Valls-Gabaud, David; Walter, Frederick M; Webb, John K<title>Abstract</title> <p>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 known. T CrB offers an excellent opportunity to test this prediction. As it will almost certainly undergo its next, once in ∼80 yr RN event between 2024 and 2026, we carried out very deep narrowband and continuum imaging to search for the predicted, piled-up ejecta of the past millennia. While nothing is detected in continuum or narrowband [O<sc>iii</sc>] images, a ∼30 pc diameter, faint nebulosity surrounding T CrB is clearly present in deep H<italic>α</italic>, [N<sc>ii</sc>], and [S<sc>ii</sc>] narrowband Condor Array Telescope imagery. We predict that these newly detected nebulosities, as well as the recent ejecta that have not yet reached the super-remnant, are far too optically thin to capture all but a tiny fraction of the photons emitted by RN flashes. We thus predict that fluorescent light echoes will<italic>not</italic>be detectable following the imminent nova flash of T CrB. Dust may be released by the T CrB red giant wind in preeruption outbursts, but we have no reliable estimates of its quantity or geometrical distribution. While we cannot predict the morphology or intensity of dust-induced continuum light echoes following the coming flash, we encourage multiepoch Hubble Space Telescope optical imaging as well as James Webb Space Telescope infrared imaging of T CrB during the year after it erupts.</p>The American Astronomical Society2024-12-1810612494The Astrophysical Journal Letters9772L482041-8205https://doi.org/10.3847/2041-8213/ad991e2407764NovaeRecurrent NovaeNational Science Foundation