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류동수

Ryu, Dongsu
Astrophysics Lab.
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dc.citation.endPage 1833 -
dc.citation.number 4 -
dc.citation.startPage 1830 -
dc.citation.title JOURNAL OF THE KOREAN PHYSICAL SOCIETY -
dc.citation.volume 49 -
dc.contributor.author Lee, Seong-Jae -
dc.contributor.author Ryu, Dongsu -
dc.date.accessioned 2023-12-22T09:41:16Z -
dc.date.available 2023-12-22T09:41:16Z -
dc.date.created 2015-08-27 -
dc.date.issued 2006-10 -
dc.description.abstract We developed a new code that calculates the evolution of the angular momentum accurately in accretion flows in a two-dimensional cylindrical geometry. With the code, supersonic accretion flows with small amounts of angular momentum were simulated. Our simulations showed that an accretion shock formed and that the structure with the shock was dynamically unstable. The instability could provide an explanation for quasi-periodic oscillations in the black holes of galactic microquasars -
dc.identifier.bibliographicCitation JOURNAL OF THE KOREAN PHYSICAL SOCIETY, v.49, no.4, pp.1830 - 1833 -
dc.identifier.issn 0374-4884 -
dc.identifier.scopusid 2-s2.0-33751068106 -
dc.identifier.uri https://scholarworks.unist.ac.kr/handle/201301/18492 -
dc.identifier.wosid 000241289800020 -
dc.language 영어 -
dc.publisher KOREAN PHYSICAL SOC -
dc.title Supersonic, rotating accretion flows around black holes in a two-dimensional cylindrical geometry -
dc.type Article -
dc.description.journalRegisteredClass scopus -
dc.subject.keywordAuthor accretion disks -
dc.subject.keywordAuthor black holes -
dc.subject.keywordAuthor hydrodynamics -
dc.subject.keywordAuthor numerical simulation -

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