Laboratory analogue of a supersonic accretion column in a binary star system

Astrophysical flows exhibit rich behaviour resulting from the interplay of different forms of energy—gravitational, thermal, magnetic and radiative. For magnetic cataclysmic variable stars, material from a late, main sequence star is pulled onto a highly magnetized (B>10 MG) white dwarf. The magn...

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Detalles Bibliográficos
Autores principales: Cross, J. E., Gregori, G., Foster, J. M., Graham, P., Bonnet-Bidaud, J. -M., Busschaert, C., Charpentier, N., Danson, C. N., Doyle, H. W., Drake, R. P., Fyrth, J., Gumbrell, E. T., Koenig, M., Krauland, C., Kuranz, C. C., Loupias, B., Michaut, C., Mouchet, M., Patankar, S., Skidmore, J., Spindloe, C., Tubman, E. R., Woolsey, N., Yurchak, R., Falize, É.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group 2016
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4910020/
https://www.ncbi.nlm.nih.gov/pubmed/27291065
http://dx.doi.org/10.1038/ncomms11899

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4910020/
https://www.ncbi.nlm.nih.gov/pubmed/27291065
http://dx.doi.org/10.1038/ncomms11899

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