A New Interpretation for the Second Peak of T Coronae Borealis Outbursts: A Tilting Disk around a Very Massive White Dwarf
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference28 articles.
1. Allen, C. W. 1973, in Astrophysical Quantities (London: Athlone), chap. 10
2. New binary parameters for the symbiotic recurrent nova T Coronae Borealis
3. The secondary outburst maximum of T Coronae Borealis - Implications for the physics of accretion disks
4. Approximations to the radii of Roche lobes
5. Updated Opal Opacities
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2. Recurrent Symbiotic Nova T Coronae Borealis before Outburst;Astronomy Letters;2023-09
3. Recurrent Symbiotic Nova T Coronae Borealis before Outburst;Письма в Астрономический журнал: Астрономия и космическая астрофизика;2023-09-01
4. The B & V light curves for recurrent nova T CrB from 1842–2022, the unique pre- and post-eruption high-states, the complex period changes, and the upcoming eruption in 2025.5 ± 1.3;Monthly Notices of the Royal Astronomical Society;2023-03-14
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