A helium-burning white dwarf binary as a supersoft X-ray source

Type Ia supernovae are cosmic distance indicators(1,2), and the main source of iron in the Universe(3,4), but their formation paths are still debated. Several dozen supersoft X-ray sources, in which a white dwarf accretes hydrogen-rich matter from a non-degenerate donor star, have been observed(5) a...

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Detalles Bibliográficos
Autores principales: Greiner, J., Maitra, C., Haberl, F., Willer, R., Burgess, J. M., Langer, N., Bodensteiner, J., Buckley, D. A. H., Monageng, I. M., Udalski, A., Ritter, H., Werner, K., Maggi, P., Jayaraman, R., Vanderspek, R.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2023
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10033417/
https://www.ncbi.nlm.nih.gov/pubmed/36949334
http://dx.doi.org/10.1038/s41586-023-05714-4

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10033417/
https://www.ncbi.nlm.nih.gov/pubmed/36949334
http://dx.doi.org/10.1038/s41586-023-05714-4

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