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Using chemical evolution models of the Milky Way disk to constrain Type Ia supernova progenitors

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Trueman, T. C. L., Pignatari, M., Cseh, B., Keegans, J. D., Côté, B., Gibson, B. K.
Formato:	Preprint
Publicado:	2025
Materias:	Solar and Stellar Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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