THREE-DIMENSIONAL NUMERICAL HYDRODYNAMIC SIMULATION OF ON- AND OFF-STATES IN MICROQUASARS AND QUASARS

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dc.contributor.authorNazarenko, V. V.
dc.contributor.authorNazarenko, S. V.
dc.date.accessioned2015-04-06T07:31:48Z
dc.date.available2015-04-06T07:31:48Z
dc.date.issued2014
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2014 . – Vol.27, I. 2.uk
dc.description.abstractAs is shown in the present computations performed using three-dimensional numerical astrophysical methods, in microquasars in the course of precession of the accretion disc blown by the donor’s wind the on- and off-states start being generated in the disc. In our case, the transition between these states takes 30-40 minutes of the orbital time. In the off-state the temperature changes discretely, i.e. such a change appears as separate sharp peaks, which almost merge with each other over time.uk
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/6223
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;V. 27, I. 2, P. 137-141.
dc.subjectclose binary systemuk
dc.subjectmicroquasarsuk
dc.subjectquasarsuk
dc.titleTHREE-DIMENSIONAL NUMERICAL HYDRODYNAMIC SIMULATION OF ON- AND OFF-STATES IN MICROQUASARS AND QUASARSuk
dc.typeArticleuk
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Odesa Astronomical Publications