Published January 1976 | Version v1
Journal article

On the formation of disk around a compact object by two-body tidal encounter

Creators

  • 1. Kyoto Univ. (Japan)

Description

Fabian, Pringle & Rees recently argued that close binary systems may be formed by two-body tidal interaction, and that these may account for observed X-ray sources near the centres of globular clusters. In this note it is shown, by making use of Woolfson's results for capture processes, that through tidal interaction, disks can be formed around single compact objects which may emit thermal X-rays for |${10}^{5}\,\sim\,{10}^{6}$| yr.

Additional details

Identifiers

Publishing Information

Journal Title
Monthly Notices of the Royal Astronomical Society
Journal Volume
174
Journal Issue
1
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
19P-20P
ISSN
0035-8711

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
7238817
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
No Abstract
Descriptors DEI
BINARY STARS; CONFIGURATION; COSMIC X-RAY SOURCES; DISTANCE; GRAVITATIONAL FIELDS; STAR EVOLUTION; TIDES; TWO-BODY PROBLEM; X RADIATION
Descriptors DEC
COSMIC RAY SOURCES; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; MANY-BODY PROBLEM; RADIATIONS; STARS

Optional Information

Notes
Short communication.; Updated automatically by Metadata and Full-Text Enrichment Agent