Tidal Effects on Stellar Evolution in Close Binaries Formed in Globular Clusters View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1988

AUTHORS

H. M. Antia , A. K. Kembhavi , A. Ray

ABSTRACT

A mechanism of forming x-ray binaries by close collision of a neutron star and a normal star in a globular cluster core (GC) was proposed by Fabian, Pringle and Rees (1975). Press and Teukolsky (1977) (PT) made detailed computaions of tidal energy deposition in the non-radial modes of a main sequence (MS) star (approximated by a n = 3 ploytrope) and two-body tidal capture cross-section. Here, we correct numerical errors in PT for the n = 3 plytrope; extend the calculation to the n = 3/2 case which better approxiamtes a fully convective low mass star most abundant in GC; we discuss the effects of tidal energy dissipation on the evolution of the MS star and the binary orbit. More... »

PAGES

671-672

Book

TITLE

The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies

ISBN

978-90-277-2665-0
978-94-015-1104-9

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-015-1104-9_153

DOI

http://dx.doi.org/10.1007/978-94-015-1104-9_153

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1028581775


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