EPISODIC ACCRETION IN PROPLANETARY DISCS AS A RESULT OF CONVECTIVE INSTABILITY

L. Maksimova, Y. Pavlyuchenkov
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Abstract

Using the model of viscous evolution of the disk and the calculation of the vertical structure, the evolution of the Keplerian disk and its morphology are investigated. The episodic nature of accretion was revealed and the effect of various initial parameters on the behavior of flashes in the protoplanetary disk was investigated.
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对流不稳定导致的前行星盘的偶发性吸积
利用盘的粘性演化模型和垂直结构的计算,研究了开普勒盘的演化及其形态。揭示了吸积的偶发性,并研究了不同初始参数对原行星盘中闪光行为的影响。
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ORBITAL COMPOSITION OF INNER BARS IN DISK GALAXIES THE ESCAPE OF ASTEROID DUST PARTICLES DUE TO SOLAR RADIATION MIDDLE AND UPPER ATMOSPHERE: PROBLEMS, TRENDS, PARTICLES COLD METHANOL FORMATION LADDER AND VISUAL EXTINCTION: TEST THE CHEMICAL MODEL THE MODIFIED TECHNIQUE FOR THE IDENTIFICATION AND STUDY OF SECULAR RESONANCES IN THE DYNAMICS OF NEAR-PLANETARY OBJECTS
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