TL;DR
This paper reviews the physical characteristics of symbiotic novae, a type of thermonuclear nova in long-period binary systems with red giant donors, and discusses their relationship within the broader symbiotic star family.
Contribution
It provides a comprehensive overview of symbiotic novae's physical properties and clarifies their position among symbiotic stars, highlighting their unique features.
Findings
Symbiotic novae are characterized by long orbital periods.
They exhibit thermonuclear activity on red giant donors.
The paper discusses their evolutionary significance.
Abstract
The symbiotic novae are thermonuclear novae in symbiotic binary systems -- interacting binaries with evolved red giant donors, and the longest orbital periods. This paper aims at presenting physical characteristics of these objects and discussing their place among the whole family of symbiotic stars.
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astronomy and Astrophysical Research · Astronomical Observations and Instrumentation