Laboratory analogue of a supersonic accretion column in a binary star system
Stationary radiative shocks are expected to form above the surface of highly-magnetized white dwarves in binary systems, but this cannot be resolved by telescopes. Here, the authors report a laboratory experiment showing the evolution of a reverse shock when both ionization and radiative losses are...
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2016
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oai:doaj.org-article:e7e067a3843f4aaa843c5594b4089ab62021-12-02T16:49:40ZLaboratory analogue of a supersonic accretion column in a binary star system10.1038/ncomms118992041-1723https://doaj.org/article/e7e067a3843f4aaa843c5594b4089ab62016-06-01T00:00:00Zhttps://doi.org/10.1038/ncomms11899https://doaj.org/toc/2041-1723Stationary radiative shocks are expected to form above the surface of highly-magnetized white dwarves in binary systems, but this cannot be resolved by telescopes. Here, the authors report a laboratory experiment showing the evolution of a reverse shock when both ionization and radiative losses are important.J. E. CrossG. GregoriJ. M. FosterP. GrahamJ. -M. Bonnet-BidaudC. BusschaertN. CharpentierC. N. DansonH. W. DoyleR. P. DrakeJ. FyrthE. T. GumbrellM. KoenigC. KraulandC. C. KuranzB. LoupiasC. MichautM. MouchetS. PatankarJ. SkidmoreC. SpindloeE. R. TubmanN. WoolseyR. YurchakÉ. FalizeNature PortfolioarticleScienceQENNature Communications, Vol 7, Iss 1, Pp 1-7 (2016) |
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Science Q J. E. Cross G. Gregori J. M. Foster P. Graham J. -M. Bonnet-Bidaud C. Busschaert N. Charpentier C. N. Danson H. W. Doyle R. P. Drake J. Fyrth E. T. Gumbrell M. Koenig C. Krauland C. C. Kuranz B. Loupias C. Michaut M. Mouchet S. Patankar J. Skidmore C. Spindloe E. R. Tubman N. Woolsey R. Yurchak É. Falize Laboratory analogue of a supersonic accretion column in a binary star system |
| description |
Stationary radiative shocks are expected to form above the surface of highly-magnetized white dwarves in binary systems, but this cannot be resolved by telescopes. Here, the authors report a laboratory experiment showing the evolution of a reverse shock when both ionization and radiative losses are important. |
| format |
article |
| author |
J. E. Cross G. Gregori J. M. Foster P. Graham J. -M. Bonnet-Bidaud C. Busschaert N. Charpentier C. N. Danson H. W. Doyle R. P. Drake J. Fyrth E. T. Gumbrell M. Koenig C. Krauland C. C. Kuranz B. Loupias C. Michaut M. Mouchet S. Patankar J. Skidmore C. Spindloe E. R. Tubman N. Woolsey R. Yurchak É. Falize |
| author_facet |
J. E. Cross G. Gregori J. M. Foster P. Graham J. -M. Bonnet-Bidaud C. Busschaert N. Charpentier C. N. Danson H. W. Doyle R. P. Drake J. Fyrth E. T. Gumbrell M. Koenig C. Krauland C. C. Kuranz B. Loupias C. Michaut M. Mouchet S. Patankar J. Skidmore C. Spindloe E. R. Tubman N. Woolsey R. Yurchak É. Falize |
| author_sort |
J. E. Cross |
| title |
Laboratory analogue of a supersonic accretion column in a binary star system |
| title_short |
Laboratory analogue of a supersonic accretion column in a binary star system |
| title_full |
Laboratory analogue of a supersonic accretion column in a binary star system |
| title_fullStr |
Laboratory analogue of a supersonic accretion column in a binary star system |
| title_full_unstemmed |
Laboratory analogue of a supersonic accretion column in a binary star system |
| title_sort |
laboratory analogue of a supersonic accretion column in a binary star system |
| publisher |
Nature Portfolio |
| publishDate |
2016 |
| url |
https://doaj.org/article/e7e067a3843f4aaa843c5594b4089ab6 |
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