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To Be or not to Be: the role of rotation in modeling Galactic Be X-ray Binaries

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Rocha, Kyle Akira, Kalogera, Vicky, Doctor, Zoheyr, Andrews, Jeff J., Sun, Meng, Gossage, Seth, Bavera, Simone S., Fragos, Tassos, Kovlakas, Konstantinos, Kruckow, Matthias U., Misra, Devina, Srivastava, Philipp M., Xing, Zepei, Zapartas, Emmanouil
Formato:	Preprint
Publicado:	2024
Materias:	High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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