The secondary maximum of T CrB caused by irradiation of the red giant by a cooling white dwarf
| Autor: | Munari, Ulisse |
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| Rok vydání: | 2023 |
| Předmět: | |
| Zdroj: | published in RNAAS, 7, 251, (2023) |
| Druh dokumentu: | Working Paper |
| DOI: | 10.3847/2515-5172/ad0f26 |
| Popis: | Both the 1866 and 1946 outbursts of the recurrent symbiotic nova T CrB have displayed a mysterious secondary maximum peaking in brightness ~5 months past the primary one. Common to all previous modeling attempts was the rejection of plain irradiation of the red giant (RG), on the basis that the secondary maximum of T CrB would have been out of phase with the transit at superior conjunction of the RG. Implicit to this line of reasoning is the assumption of a constant temperature for the white dwarf (WD) irradiating the red giant. I show by radiative modeling that irradiation of the RG by a cooling WD nicely reproduces the photometric evolution of the secondary maximum, both in terms of brightness and color, removes the phasing offset, and provides a straightforward explanation that will be easy to test at the next and imminent outburst. Comment: correcting a label in Figure 1 |
| Databáze: | arXiv |
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