Please use this identifier to cite or link to this item: http://dspace.onu.edu.ua:8080/handle/123456789/9803
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dc.contributor.authorNazarenko, V. V.-
dc.contributor.authorNazarenko, S. V.-
dc.date.accessioned2017-05-18T11:09:51Z-
dc.date.available2017-05-18T11:09:51Z-
dc.date.issued2016-
dc.identifier.citationOdessa Astronomical publications = Одесские астрономические публикации = Одеські астрономічні публікаціїuk
dc.identifier.urihttp://dspace.onu.edu.ua:8080/handle/123456789/9803-
dc.description.abstractIn the present research we have calculated 3D numerical hydrodynamical simulations of a radiation-driven jet launch and disappearing over low/hard state. The calculations show that the jet launch occurs at the beginning of the low/hard state over 10-30 minutes of the orbital time. The jet disappearing occurs over the short time scale (of the order of 10-30 minutes of the orbital time) at the end of the low/hard state. The calculations also show that the temperature near the accretor is increased in 100-200 times over low/hard state relatively high/soft. The mass accretion rate in the disc is anti-correlated with the temperature near the accretor in our calculations.uk
dc.language.isoenuk
dc.publisherОдеський національний університет імені І. І. Мечниковаuk
dc.relation.ispartofseries;Vol. 29.-
dc.subjectStars: binaries - starsuk
dc.subjectjets - methodsuk
dc.subjectnumerical - hydrodynamicsuk
dc.title3D numerical hydrodynamical simulations of a radiation-driven jet launch and disappearing over low/hard stateuk
dc.typeArticleuk
Appears in Collections:Odessa Astronomical Publications

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