Cover Image

Hydrodynamic moving-mesh simulations of the common envelope phase in binary stellar systems

Show other versions (1)

The common envelope (CE) phase is an important stage in binary stellar evolution. It is needed to explain many close binary stellar systems, such as cataclysmic variables, SN Ia progenitors, or X-ray binaries. To form the resulting close binary, the initial orbit has to shrink, thereby transferring...

Full description

Saved in:
Bibliographic Details
Main Authors: Ohlmann, Sebastian T. (Author) , Röpke, Friedrich (Author) , Springel, Volker (Author)
Format: Article (Journal)
Language:English
Published: 2015 December 30
In: The astrophysical journal. Part 2, Letters
Year: 2016, Volume: 816, Issue: 1
ISSN:2041-8213
DOI:10.3847/2041-8205/816/1/L9
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.3847/2041-8205/816/1/L9
Verlag, kostenfrei, Volltext: http://stacks.iop.org/2041-8205/816/i=1/a=L9
Get full text
Author Notes:Sebastian T. Ohlmann, Friedrich K. Röpke, Rüdiger Pakmor, and Volker Springel
Search Result 1
Cover Image

Hydrodynamic moving-mesh simulations of the common envelope phase in binary stellar systems by Ohlmann, Sebastian T. (Author) , Röpke, Friedrich (Author) , Springel, Volker (Author) ,


Get full text
Article (Journal) Chapter/Article Online Resource

Saved in:
Show all versions (2)

Similar Items