Binary fission in damped rotating polytropes
Description
The forms of equilibrium and the mode of fission of damped differentially-rotating polytropes are calculated using the SPH method. The damping used conserves total angular momentum and angular momentum per unit mass. The equilibrium forms are similar to the classical liquid, viscous sequences with a transition from axisymmetric to approximately ellipsoidal forms when T/vertical bar W vertical bar approximately 0.14. Sequences with n = 0.5 end by fission into two condensed bodies which form a close binary. Sequences with n = 1.5 undergo a fission which produces a stream with approximately 0.25 of the total mass. The accuracy of the calculations has been estimated by running sequences with different particle numbers, initial particle positions and variations in the choice of the smoothing length. These parameters produce sequences which are very similar, up to the point of fission, but the details of the binary (or stream) vary widely. (author)
Additional details
Identifiers
Publishing Information
- Journal Title
- Monthly Notices of the Royal Astronomical Society
- Journal Volume
- 184
- Journal Issue
- 3
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 481-499
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 9413122
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANGULAR MOMENTUM; BINARY STARS; DAMPING; EQUILIBRIUM; ORIGIN; ROTATION; STAR EVOLUTION; STAR MODELS
- Descriptors DEC
- MATHEMATICAL MODELS; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent