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류동수

Ryu, Dongsu
Astrophysics Lab.
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dc.citation.endPage 618 -
dc.citation.number 2 -
dc.citation.startPage 603 -
dc.citation.title ASTROPHYSICAL JOURNAL -
dc.citation.volume 339 -
dc.contributor.author Chiang, Wei-Hwan -
dc.contributor.author Ryu, Dongsu -
dc.contributor.author Vishniac, Ethan T. -
dc.date.accessioned 2023-12-22T13:10:12Z -
dc.date.available 2023-12-22T13:10:12Z -
dc.date.created 2015-08-27 -
dc.date.issued 1989-04 -
dc.description.abstract The evolution of the intergalactic medium (IGM) in a cold dark matter-dominated universe is studied. The dark matter is approximated as a pressureless ideal fluid while the IGM is approximated as an ordinary fluid. Several three-dimensional numerical simulations were carried out to trace the evolution of the model universe from z of about 100 to the present time. It is found that the growth of the rms density fluctuations in the IGM is greatly reduced during the period of heating, but it picks up at late times as gravity dominates again. -
dc.identifier.bibliographicCitation ASTROPHYSICAL JOURNAL, v.339, no.2, pp.603 - 618 -
dc.identifier.doi 10.1086/167321 -
dc.identifier.issn 0004-637X -
dc.identifier.uri https://scholarworks.unist.ac.kr/handle/201301/18568 -
dc.identifier.url http://adsabs.harvard.edu/doi/10.1086/167321 -
dc.identifier.wosid A1989U094900002 -
dc.language 영어 -
dc.publisher IOP PUBLISHING LTD -
dc.title EVOLUTION OF THE INTERGALACTIC MEDIUM IN A COLD DARK MATTER-DOMINATED UNIVERSE -
dc.type Article -
dc.description.journalRegisteredClass scopus -

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