Published January 1976
| Version v1
Journal article
On the formation of disk around a compact object by two-body tidal encounter
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