Massive binary mergers and thorne-zytkow objects
Some 10% of all massive stars are predicted to merge completely with a companion star. Here we review the different types of mergers and how they may produce unusual objects such as the anomalous progenitor of SN 1987A, gamma-ray burst sources and Thorne-Zytkow objects.
المؤلف الرئيسي: | Podsiadlowski, P |
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التنسيق: | Conference item |
منشور في: |
2007
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مواد مشابهة
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THE FATE OF THORNE-ZYTKOW OBJECTS
حسب: Podsiadlowski, P, وآخرون
منشور في: (1994) -
The structure and evolution of Thorne-Zytkow objects
حسب: Podsiadlowski, P
منشور في: (1996) -
THE STRUCTURE AND EVOLUTION OF THORNE-ZYTKOW OBJECTS
حسب: Cannon, R, وآخرون
منشور في: (1992) -
Rethinking Thorne–Żytkow Object Formation: Assembly via Common Envelope in Field Binaries
حسب: Rosa Wallace Everson, وآخرون
منشور في: (2024-01-01) -
GRBs from Collapse of Thorne–Żytkow–like Objects as the Aftermath of WD-NS Coalescence
حسب: Zong-kai Peng, وآخرون
منشور في: (2024-01-01)