Symbiotic novae
Abstract
(Invited Review) According to modern definition, a symbiotic nova is an otherwise normal nova (i.e. powered by explosive thermonuclear burning) that erupts within a symbiotic star, which is a binary where a WD accretes from a cool giant companion. Guided primarily by the very well observed eruptions of RS Oph in 2006 and 2021, and that of V407 Cyg in 2010, we investigate the main multi-wavelength properties of symbiotic novae and their relation to classical novae, and propose a 3D model structure that identifies the emitting source location for hard and supersoft X-rays, radio syncrothron and thermal, permitted and forbidden emission lines. Very few symbiotic novae are known in the Galaxy, and we compile a revised catalog based on firm astrometric identification. The exciting prospect of an imminent new outburst of T CrB is also discussed.
Keywords
Cite
@article{arxiv.2412.20499,
title = {Symbiotic novae},
author = {Ulisse Munari},
journal= {arXiv preprint arXiv:2412.20499},
year = {2024}
}
Comments
Invited review, in press, Proceedings of Kopal 2024 conference "Binary and Multiple Stars", Litomysl (Czech Rep.,) 9-13 September 2024