The Reason for the Occurrence of W-type Contact Binaries
For more than half a century, the puzzling W-type phenomenon in contact binaries has challenged astrophysicists. In these systems, the less massive component exhibits a higher surface temperature than its more massive companion, which is a reversal of the typical A-type configuration, where the more...
I tiakina i:
| Ngā kaituhi matua: | , , , |
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| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
IOP Publishing
2025-01-01
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| Rangatū: | The Astrophysical Journal Supplement Series |
| Ngā marau: | |
| Urunga tuihono: | https://doi.org/10.3847/1538-4365/ae21ce |
| Ngā Tūtohu: |
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