Delayed and Displaced: The Impact of Binary Interactions on Core-collapse SN Feedback

Core-collapse supernova feedback models in hydrodynamical simulations typically assume that all stars evolve as single stars. However, the majority of massive stars are formed in binaries and multiple systems, where interactions with a companion can affect stars’ subsequent evolution and kinematics....

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Xehetasun bibliografikoak

Egile Nagusiak:	Tom Wagg, Julianne J. Dalcanton, Mathieu Renzo, Katelyn Breivik, Matthew E. Orr, Adrian M. Price-Whelan, Akaxia Cruz, Alyson Brooks, Ulrich P. Steinwandel, Eric C. Bellm
Formatua:	Artigo
Hizkuntza:	Inglês
Argitaratua:	IOP Publishing 2025-01-01
Saila:	The Astronomical Journal
Gaiak:	Binary stars Stellar evolution Stellar feedback Core-collapse supernovae Galaxy dynamics Hydrodynamical simulations
Sarrera elektronikoa:	https://doi.org/10.3847/1538-3881/adf55e
Etiketak:	Etiketa erantsi Etiketarik gabe, Izan zaitez lehena erregistro honi etiketa jartzen!