Please use this identifier to cite or link to this item: http://dspace.onu.edu.ua:8080/handle/123456789/6223
Title: THREE-DIMENSIONAL NUMERICAL HYDRODYNAMIC SIMULATION OF ON- AND OFF-STATES IN MICROQUASARS AND QUASARS
Authors: Nazarenko, V. V.
Nazarenko, S. V.
Citation: Odessa Astronomical Publications
Issue Date: 2014
Publisher: Astroprint
Keywords: close binary system
microquasars
quasars
Series/Report no.: ;V. 27, I. 2, P. 137-141.
Abstract: As 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.
Description: Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2014 . – Vol.27, I. 2.
URI: http://dspace.onu.edu.ua:8080/handle/123456789/6223
Appears in Collections:Odessa Astronomical Publications

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