Published June 1, 1976
| Version v1
Journal article
Discovery of a 283-second periodic variation in the X-ray source 3U 0900--40
Creators
- 1. Department of Physics and Center for Space Research, Massachusetts Institute of Technology
Description
A 283 s periodic pulsation in the X-ray system 3U 0900--40 has been discovered during observations by the SAS-3 X-ray observatory. Pulse profiles of the 283 s periodicity are presented in five energy intervals covering the range 1--30 keV for the period 1975 July 19.4--23.9. The averaged profile is relatively simple at higher energies and is markedly more complex at lower energies. The peak 1--40 keV intensity observed for the source is 1.2 x 10-8 ergs cm-2 s-1, which corresponds to a luminosity of 2.1 x 1036 ergs s-1 at a distance of 1.2 kpc. A search for soft X-ray emission (E<1 keV) yielded upper limits of 2 x 10-11 and 5 x 10-11 ergs cm-2 s-1 in the energy intervals 0.16--0.28 keV and 0.5--0.7 keV, respectively
Additional details
Identifiers
- DOI
- 10.1086/182142;
Publishing Information
- Journal Title
- The Astrophysical Journal
- Journal Volume
- 206
- Journal Issue
- 2
- Series
- Astrophys. J., Lett.
- Journal Page Range
- L99
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 8285204
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BINARY STARS; COSMIC X-RAY SOURCES; NEUTRON STARS; PULSARS; PULSATIONS; SOFT X RADIATION; VARIABLE STARS
- Descriptors DEC
- COSMIC RADIO SOURCES; COSMIC RAY SOURCES; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; RADIATIONS; STARS; X RADIATION
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent