Dynamical portrait of the Lixiaohua asteroid family-Reference-Cited by-同舟云学术

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Dynamical portrait of the Lixiaohua asteroid family

Published:2010-03-12 Issue:1-2 Volume:107 Page:35-49
ISSN:0923-2958
Container-title:Celestial Mechanics and Dynamical Astronomy
language:en
Short-container-title:Celest Mech Dyn Astr

Author:

Novaković B.,Tsiganis K.,Knežević Z.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics,Applied Mathematics,Computational Mathematics,Mathematical Physics,Modelling and Simulation

Link

http://link.springer.com/content/pdf/10.1007/s10569-010-9263-9.pdf

Reference35 articles.

1. Baer J., Chesley S.R.: Astrometric masses of 21 asteroids and an integrated asteroid ephemeris. Cel. Mech. Dyn. Astron. 100, 27–42 (2008)

2. Bendjoya Ph., Zappalà V.: Asteroid family identification. In: Bottke, W.F., Cellino, A., Paolicchi, P., Binzel, R.P. (eds) Asteroids III, pp. 613–618. University of Arizona Press, Tucson (2002)

3. Bottke W.F., Vokrouhlický D., Rubincam D.P., Nesvorný D.: The Yarkovsky and Yorp effects: implications for asteroid dynamics. Annu. Rev. Earth. Planet. Sci. 34, 157–191 (2006)

4. Carpino, M., Knežević, Z.: Asteroid mass determination: (1) Ceres. In: Ferraz-Mello, S., Morando, B., Arlot, J.-E. (eds.) Dynamics, ephemerides, and astrometry of the solar system: proceedings of the 172nd symposium of the IAU, pp. 203–206 (1996)

5. Carruba V., Burns J.A., Bottke W.F., Nesvorný D.: Orbital evolution of the Gefion and Adeona asteroid families: close encounters with massive asteroids and the Yarkovsky effect. Icarus 162, 308–327 (2003)

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