Measuring the density structure of an accretion hot spot

Magnetospheric accretion models predict that matter from protoplanetary disks accretes onto stars via funnel flows, which follow stellar magnetic field lines and shock on the stellar surfaces(1–3), leaving hot spots with density gradients(4–6). Previous work has provided observational evidence of va...

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Detalles Bibliográficos
Autores principales: Espaillat, C. C., Robinson, C. E., Romanova, M. M., Thanathibodee, T., Wendeborn, J., Calvet, N., Reynolds, M., Muzerolle, J.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2021
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8410598/
https://www.ncbi.nlm.nih.gov/pubmed/34471274
http://dx.doi.org/10.1038/s41586-021-03751-5

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8410598/
https://www.ncbi.nlm.nih.gov/pubmed/34471274
http://dx.doi.org/10.1038/s41586-021-03751-5

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