Published July 15, 1974
| Version v1
Journal article
OSO-7 observations of Circinus X-1
Creators
- 1. Department of Physics and Center for Space Research, Massachusetts Institute of Technology, Cambridge
Description
We present data from six observations with the MIT X-ray detectors on the 0S0-7. The results for one 5d interval rule out the 12 d.288 binary eclipse period proposed by Jones, Tananbaum, and Giacconi for this source. The average spectrum is considerably steeper than those of the established eclipsing binaries. Subject headings: binaries - X-ray sources
Additional details
Additional titles
- Augmented title (English)
- Gaunt factor, eclipse period
Identifiers
- DOI
- 10.1086/181552;
Publishing Information
- Journal Title
- The Astrophysical Journal
- Journal Volume
- 191
- Journal Issue
- 2
- Series
- Astrophys. J., Lett.
- Journal Page Range
- L75
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 6159256
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BINARY STARS; BREMSSTRAHLUNG; COSMIC X-RAY SOURCES; ECLIPSE; SPECTRA; VARIATIONS; X RADIATION
- Descriptors DEC
- COSMIC RAY SOURCES; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; RADIATIONS; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent