Orbital stability near the (87) Sylvia system-Reference-Cited by-同舟云学术

Orbital stability near the (87) Sylvia system

Published:2019-04-12 Issue:2 Volume:486 Page:2557-2569
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Aljbaae S¹,Chanut T G G¹,Prado A F B A¹,Carruba V²^ORCID,Hussmann H³,Souchay J⁴,Sanchez D M¹^ORCID

Affiliation:

1. Division of Space Mechanics and Control, INPE, C.P. 515, 12227-310 São José dos Campos, SP, Brazil

2. School of Natural Sciences and Engineering, São Paulo State University (UNESP), 12516-410 Guaratinguetá, SP, Brazil

3. DLR Institute of Planetary Research, Rutherfordstr. 2, D-2489 Berlin, Germany

4. SYRTE, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Univ. Paris 06, LNE, 61 avenue de l’Observatoire, F-75014 Paris, Fr

Funder

National Council for Scientific and Technological Development

São Paulo State Science Foundation

Coordination for the Improvement of Higher Education Personnel

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz998/28370017/stz998.pdf

Reference45 articles.

1. The dynamical environment of asteroid 21 Lutetia according to different internal models

2. Multiple asteroid systems (45) Eugenia and (87) Sylvia: Sensitivity to external and internal perturbations

3. Physical and dynamical properties of the main belt triple Asteroid (87) Sylvia

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