Wide B-type hot subdwarf binaries
Context. Long-period binary systems containing a B-type hot subdwarf (sdB) and a main sequence (MS) companion are thought to originate from binary interactions involving stable mass transfer from the red giant, which is the progenitor of the sdB, to the MS companion. However, despite the recent prog...
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| Päätekijät: | , , , |
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| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
EDP Sciences
2026-06-01
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| Sarja: | Astronomy & Astrophysics |
| Aiheet: | |
| Linkit: | https://www.aanda.org/articles/aa/full_html/2026/06/aa59320-26/aa59320-26.html |
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