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Simplified method for the identification of low mass ratio contact binary systems that are potential red nova progenitors

Surjit S. Wadhwa, Ain Y. De Horta, M. D. Filipović, N. F. H. Tothill, Б. Арбутина, J. Petrović, G. Djurašević

2022Journal of Astrophysics and Astronomy10 citationsDOI

Topics & Concepts

PhysicsNova (rocket)Contact binaryAstrophysicsBinary numberIdentification (biology)Binary systemBinary starBiologyStarsBotanyAerospace engineeringArithmeticEngineeringMathematicsAstrophysical Phenomena and ObservationsStellar, planetary, and galactic studiesGamma-ray bursts and supernovae
Simplified method for the identification of low mass ratio contact binary systems that are potential red nova progenitors | Litcius