1![FOR RELEASE: 9:20 AM EST, January 7, 2002 ORBITAL STABILITY OF EARTH-LIKE PLANETS IN STELLAR HABITABLE ZONES Long-term orbital stability of Earth-like planets in stellar habitable zones is necessary for the evolution of FOR RELEASE: 9:20 AM EST, January 7, 2002 ORBITAL STABILITY OF EARTH-LIKE PLANETS IN STELLAR HABITABLE ZONES Long-term orbital stability of Earth-like planets in stellar habitable zones is necessary for the evolution of](https://www.pdfsearch.io/img/f448cb51512c36bb9c4bf73828b0792e.jpg) | Add to Reading ListSource URL: www.uta.eduLanguage: English - Date: 2015-06-10 15:36:23
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2![Transverse stability issues in Hamiltonian partial differential equations Nikolay Tzvetkov (University Cergy-Pontoise) The famous Korteweg- de Vries (KdV) equation ∂t u + u∂x u + ∂x3 u = 0 is a one dimensional asym Transverse stability issues in Hamiltonian partial differential equations Nikolay Tzvetkov (University Cergy-Pontoise) The famous Korteweg- de Vries (KdV) equation ∂t u + u∂x u + ∂x3 u = 0 is a one dimensional asym](https://www.pdfsearch.io/img/0564fe6a64978c8efe33906bedcafe66.jpg) | Add to Reading ListSource URL: www.7ecm.deLanguage: English - Date: 2016-06-10 05:01:15
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3![JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 116, E03010, doi:2010JE003652, 2011 Effects of orbital evolution on lunar ice stability Matthew A. Siegler,1 Bruce G. Bills,2 and David A. Paige1 Received 13 May 2010; revis JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 116, E03010, doi:2010JE003652, 2011 Effects of orbital evolution on lunar ice stability Matthew A. Siegler,1 Bruce G. Bills,2 and David A. Paige1 Received 13 May 2010; revis](https://www.pdfsearch.io/img/250425907715e585eda0045b02e550e3.jpg) | Add to Reading ListSource URL: diviner.ucla.eduLanguage: English - Date: 2014-10-30 17:13:24
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4![Stability of Nonlinear Systems By Guanrong Chen Department of Electronic Engineering City University of Hong Kong Stability of Nonlinear Systems By Guanrong Chen Department of Electronic Engineering City University of Hong Kong](https://www.pdfsearch.io/img/baa0e80e76f3a114deeb6a2a6e6371e8.jpg) | Add to Reading ListSource URL: www.ee.cityu.edu.hkLanguage: English - Date: 2009-10-04 02:52:38
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5![Orbital stability for NLS Jordan Bell Department of Mathematics, University of Toronto April 3, 2014 Let n = 3, and take p < 43 . Some of the material we will present for general Orbital stability for NLS Jordan Bell Department of Mathematics, University of Toronto April 3, 2014 Let n = 3, and take p < 43 . Some of the material we will present for general](https://www.pdfsearch.io/img/19ed262345e51e66978e69958a32d503.jpg) | Add to Reading ListSource URL: individual.utoronto.caLanguage: English - Date: 2014-04-03 12:52:33
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6![J. Phys. Chem. B 2004, 108, 17337 Why Does Disubstituted Hexamolybdate with Arylimido Prefer to Form an Orthogonal Derivative? Analysis of Stability, Bonding Character, and Electronic Properties on J. Phys. Chem. B 2004, 108, 17337 Why Does Disubstituted Hexamolybdate with Arylimido Prefer to Form an Orthogonal Derivative? Analysis of Stability, Bonding Character, and Electronic Properties on](https://www.pdfsearch.io/img/6f4ca016595a004d51d9aba4a3be521e.jpg) | Add to Reading ListSource URL: yangtze.hku.hkLanguage: English - Date: 2010-12-19 08:35:07
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7![J. Phys. Chem. B 2004, 108, [removed]17337 Why Does Disubstituted Hexamolybdate with Arylimido Prefer to Form an Orthogonal Derivative? Analysis of Stability, Bonding Character, and Electronic Properties on J. Phys. Chem. B 2004, 108, [removed]17337 Why Does Disubstituted Hexamolybdate with Arylimido Prefer to Form an Orthogonal Derivative? Analysis of Stability, Bonding Character, and Electronic Properties on](https://www.pdfsearch.io/img/69ab7e6a400facf5c0e2320eedd75e83.jpg) | Add to Reading ListSource URL: yangtze.hku.hkLanguage: English - Date: 2010-12-19 08:35:07
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8![NONLINEAR DYNAMICS AND SYSTEMS THEORY An International Journal of Research and Surveys Volume 1 Number 2
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9![DYNAMICS OF KDV SOLITONS IN THE PRESENCE OF A SLOWLY VARYING POTENTIAL JUSTIN HOLMER Abstract. We study the dynamics of solitons as solutions to the perturbed KdV (pKdV) equation ∂t u = −∂x (∂x2 u + 3u2 − bu), DYNAMICS OF KDV SOLITONS IN THE PRESENCE OF A SLOWLY VARYING POTENTIAL JUSTIN HOLMER Abstract. We study the dynamics of solitons as solutions to the perturbed KdV (pKdV) equation ∂t u = −∂x (∂x2 u + 3u2 − bu),](https://www.pdfsearch.io/img/e80bbca7fa45f67548a91bb73f2dbc4e.jpg) | Add to Reading ListSource URL: www.math.brown.eduLanguage: English - Date: 2010-12-31 00:02:51
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10![RESEARCH ARTICLE The Origin of Chaos in the Outer Solar System N. Murray1 and M. Holman2 Classical analytic theories of the solar system indicate that it is stable, but RESEARCH ARTICLE The Origin of Chaos in the Outer Solar System N. Murray1 and M. Holman2 Classical analytic theories of the solar system indicate that it is stable, but](https://www.pdfsearch.io/img/66b61ef063974f81172823fa4ae5e4af.jpg) | Add to Reading ListSource URL: www.cita.utoronto.caLanguage: English - Date: 2000-06-14 12:17:18
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