The use of heterogeneous mechanics for modeling a gas-dust protoplanetary disk: 1. The laminar stage of subdisk formation-Reference-Cited by-同舟云学术

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The use of heterogeneous mechanics for modeling a gas-dust protoplanetary disk: 1. The laminar stage of subdisk formation

Published:2020 Issue:39 Volume: Page:1-44
ISSN:2071-2898
Container-title:Keldysh Institute Preprints
language:
Short-container-title:KIAM Prepr.

Author:

Kolesnichenko Aleksandr Vladimirovich¹^ORCID

Affiliation:

1. Keldysh Institute of Applied Mathematics

Publisher

Keldysh Institute of Applied Mathematics

Subject

General Medicine

Reference90 articles.

1. Сафронов В.С. Современное состояние теории происхождения Земли//Физика Земли. 1982. № 6. С. 5-24.

2. Шмидт О.Ю. Четыре лекции о происхождении Земли. Изд. 3, доп. М.: Изд-во АН СССР. 1957. 140 с.

3. Сафронов В.С. Эволюция допланетного облака и образование Земли и планет. М.: Наука. 1969. 244 с.

4. Goldrich P., Ward W.R. The formation of planetesimals// Astrophys. J. 1973. V.183. № 3. P. 1051-1061.

5. Makalkin A.B. Radial compaction of the dust subdisk in a protoplanetary disk as possible way to gravitational instability//Lunar Planet. Sci. 1994. V.25. P. 827-828.

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1. The use of heterogeneous mechanics for modeling a gas-dust protoplanetary disk: II. The laminar stage of subdisk formation;Keldysh Institute Preprints;2021

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