Influence of the water content in protoplanetary discs on planet migration and formation

E-ISSN： 1432-0746|590|issue|A101-A101

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.590, Iss.issue, 2016-05, pp. : A101-A101

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

Revisiting the “radial-drift barrier” of planet formation and its relevance in observed protoplanetary discs⋆

By Laibe G. Gonzalez J.-F. Maddison S. T.

Astronomy & Astrophysics, Vol. 537, Iss. issue, 2012-01 ,pp. : A61-A61

Edp Sciences

Access to resources Recommend Favorite

Gas composition of the main volatile elements in protoplanetary discs and its implication for planet formation

By Thiabaud A. Marboeuf U. Alibert Y. Leya I. Mezger K.

Astronomy & Astrophysics, Vol. 574, Iss. issue, 2015-02 ,pp. : A138-A138

Edp Sciences

Access to resources Recommend Favorite

Range of outward migration and influence of the disc’s mass on the migration of giant planet cores

By Bitsch B. Kley W.

Astronomy & Astrophysics, Vol. 536, Iss. issue, 2011-12 ,pp. : A77-A77

Edp Sciences

Access to resources Recommend Favorite

Migration and giant planet formation

Astronomy & Astrophysics, Vol. 417, Iss. 1, 2004-04 ,pp. : L25-L28

Edp Sciences

Access to resources Recommend Favorite

Planet migration in three-dimensional radiative discs

Astronomy & Astrophysics, Vol. 506, Iss. 2, 2009-11 ,pp. : 971-987

Edp Sciences

Access to resources Recommend Favorite