SIMULATED IMPACTS TO NON-MAGNETIC CATACLYSMIC VARIABLE DISKS
Dust has recently been found to be prevalent in compact binaries such as non-magnetic Cataclysmic Variable systems. As a possible source of this dust is from solid bodies, we explore impacts to non-magnetic Cataclysmic Variable disks. We use three-dimensional Smoothed Particle Hydrodynamic simulatio...
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Veröffentlicht in: | Publications of The Korean Astronomical Society 2015-09, Vol.30 (2), p.179-182 |
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Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
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