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When and Why Formation of Large Bodies in Circumstellar Discs Could Take Place? Full article

Conference Instabilities and Structures in Proto-Planetary Disks
17-20 Sep 2012 , Marseille
Source Instabilities and Structures in Proto-Planetary Disks
Compilation, 2013. ISBN 9782759809837.
Journal EPJ Web of Conferences
, E-ISSN: 2100-014X
Output data Year: 2013, Volume: 46, Article number : 07004, Pages count : 8 DOI: 10.1051/epjconf/20134607004
Authors Snytnikov Valeriy N. 1 , Stoyanovskaya Olga P. 1 , Stadnichenko Olga A. 1
Affiliations
1 Boreskov Institute of Catalysis, 630090, Pr.Academika Lavrentieva, 5, Novosibirsk, Russia

Abstract: We outlined the scenario of the planetary system formation, where large bodies are formed on the stage of massive discs. On this stage the whole of factors: chemical composition, chemical catalytic reactions, the disc self- gravitation, the increased ratio of solids to gas surface density, adiabatic gas cooling provides favorable conditions for gravitational instabilities development. Gravitational instabilities in multiphase medium can lead to planetesimal and planetary embryo formation.
Cite: Snytnikov V.N. , Stoyanovskaya O.P. , Stadnichenko O.A.
When and Why Formation of Large Bodies in Circumstellar Discs Could Take Place?
In compilation Instabilities and Structures in Proto-Planetary Disks. 2013. – ISBN 9782759809837. DOI: 10.1051/epjconf/20134607004 WOS Scopus РИНЦ ANCAN OpenAlex
Files: Full text from publisher
Dates:
Published online: Apr 11, 2013
Identifiers:
Web of science: WOS:000319936900030
Scopus: 2-s2.0-84876229342
Elibrary: 20432890
Chemical Abstracts: 2013:655671
Chemical Abstracts (print): 161:43142
OpenAlex: W2110051915
Citing:
DB Citing
Web of science 1
Scopus 1
Elibrary 1
OpenAlex 1
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