Published March 1, 1976
| Version v1
Journal article
Studies of the average pulse shape of Centaurus X-3 in the 2--20 keV range
Creators
- 1. Center for Astrophysics, Harvard College Observatory/Smithsonian Astrophysical Observatory
Description
An analysis is reported of the average pulse shape of Cen X-3 versus energy (2--20 keV) on time scales of hours to days derived from Uhuru observations during 1971 May 5--7 and 1971 December 18--20. The pulsed fraction varied with energy from 0.42 +- 0.02 to 0.80 +- 0.10 over the 2--20 keV range. The 2--6 keV pulsed fraction did not show statistically significant variations (>2 sigma) over the phase of the 2.087 day eclipse cycle. Individual measurements of the 2--6 keV pulsed fraction ranged from 0.45--0.56
Additional details
Identifiers
- DOI
- 10.1086/154201;
Publishing Information
- Journal Title
- The Astrophysical Journal
- Journal Volume
- 204
- Journal Issue
- 2
- Series
- Astrophys. J.
- Journal Page Range
- 548
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 7267019
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC X-RAY SOURCES; MASS; NEUTRON STARS; PULSES; SCATTERING; TEMPERATURE DEPENDENCE; 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