Published August 1978 | Version v1
Journal article

Binary fission in damped rotating polytropes

  • 1. Cambridge Univ. Inst. of Astronomy (UK)

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
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