Abstract
The planet formation process via direct disk fragmentation is a necessary mechanism to explain the diversity of exo-planetary systems. Examples of planetary systems which might form by disk fragmentation are HR8799 and GJ758. The formation of the planets in these systems via core accretion seems to be unlikely.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsReferences
Boley, A. C. 2009, ApJ, 695, L53
Gammie, C. F. 2001, ApJ, 553, 174
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2014 Springer International Publishing Switzerland
About this paper
Cite this paper
Tsukamoto, Y., Machida, M.N., Inutsuka, Si. (2014). The Effect of Mass Accretion for Formation and Thermal Evolution of Circumstellar Disks. In: Stamatellos, D., Goodwin, S., Ward-Thompson, D. (eds) The Labyrinth of Star Formation. Astrophysics and Space Science Proceedings, vol 36. Springer, Cham. https://doi.org/10.1007/978-3-319-03041-8_15
Download citation
DOI: https://doi.org/10.1007/978-3-319-03041-8_15
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-319-03040-1
Online ISBN: 978-3-319-03041-8
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)