The Hill stability of the possible moons of extrasolar planets

ISSN： 0035-8711

Source： Monthly Notices of the Royal Astronomical Society, Vol.406, Iss.3, 2010-08, pp. : 1918-1934

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Erratum: The Hill stability of the possible moons of extrasolar planets

By Donnison J. R.

Monthly Notices of the Royal Astronomical Society, Vol. 407, Iss. 2, 2010-09 ,pp. : 1360-1360

Oxford University Press

Access to resources Recommend Favorite

The Hill stability of triple minor planets in the Solar system

By Liu Xiaodong Baoyin Hexi Georgakarakos Nikolaos Donnison John Richard Ma Xingrui

Monthly Notices of the Royal Astronomical Society, Vol. 427, Iss. 2, 2012-12 ,pp. : 1034-1042

Oxford University Press

Access to resources Recommend Favorite

Photometric Search for Extrasolar Planets

By Schneider J.

Astrophysics and Space Science, Vol. 241, Iss. 1, 1996-01 ,pp. : 35-42

Springer Publishing Company

Access to resources Recommend Favorite

Search for extrasolar planets by polarimetry

By Ksanfomality L.

Solar System Research, Vol. 41, Iss. 4, 2007-08 ,pp. : 301-306

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite

Disks, Extrasolar Planets and Migration

By Terquem C. Papaloizou J.C.B. Nelson R.P.

Space Science Reviews, Vol. 92, Iss. 1-2, 2000-01 ,pp. : 323-340

Springer Publishing Company

Access to resources Recommend Favorite