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

Journal Title: Odessa Astronomical Publications - Year 2014, Vol 27, Issue 2

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.

Authors and Affiliations

V. V. Nazarenko, S. V. Nazarenko

Keywords

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  • EP ID EP604403
  • DOI -
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How To Cite

V. V. Nazarenko, S. V. Nazarenko (2014). THREE-DIMENSIONAL NUMERICAL HYDRODYNAMIC SIMULATION OF ON- AND OFF-STATES IN MICROQUASARS AND QUASARS. Odessa Astronomical Publications, 27(2), 137-141. https://europub.co.uk/articles/-A-604403