The critical mass ratio for W UMa-type contact binary systems
Contact binaries are close binary systems in which both components fill their inner Roche lobes so that the stars are in direct contact, and in potential mass and energy exchange. The most common such systems of low mass are the so-called W UMa-type. In the last few years, there has been a...
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| Autori principali: | , |
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Astronomical Observatory, Department of Astronomy, Belgrade
2024-01-01
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| Serie: | Serbian Astronomical Journal |
| Soggetti: | |
| Accesso online: | https://doiserbia.nb.rs/img/doi/1450-698X/2024/1450-698X2408001A.pdf |
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