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Stability of discs and planetary formation around binary systems

Grant number: 08/08679-4
Support type:Scholarships in Brazil - Post-Doctorate
Effective date (Start): January 01, 2009
Effective date (End): December 31, 2010
Field of knowledge:Engineering - Aerospace Engineering - Flight Dynamics
Principal Investigator:Othon Cabo Winter
Grantee:Rita de Cássia Domingos
Home Institution: Faculdade de Engenharia (FEG). Universidade Estadual Paulista (UNESP). Campus de Guaratinguetá. Guaratinguetá , SP, Brazil
Associated research grant:06/04997-6 - Close approach problems in orbital dynamics, AP.TEM

Abstract

The discovery of planets in multistellar systems has become an interesting field for researchers. The dynamical stability and the formation process of such planets lead to questions on their origins and dynamical evolution. The existence of stellar systems with massive disks suggests that the planetary accretion process might have being similar to systems with a single star. In the present project we are interested on the study of the stability of these protoplanetary disks around binary stars and the process of planetary formation raised from them. (AU)

Scientific publications
(References retrieved automatically from Web of Science and SciELO through information on FAPESP grants and their corresponding numbers as mentioned in the publications by the authors)
DOMINGOS, R. C.; WINTER, O. C.; IZIDORO, A. Planet formation in a triple stellar system: implications of the third star's orbital inclination. International Journal of Astrobiology, v. 14, n. 2, SI, p. 153-163, APR 2015. Web of Science Citations: 1.
DOMINGOS, R. C.; WINTER, O. C.; CARRUBA, V. Mean motion resonances and the stability of a circumbinary disk in a triple stellar system. Astronomy & Astrophysics, v. 544, AUG 2012. Web of Science Citations: 2.

Please report errors in scientific publications list by writing to: cdi@fapesp.br.