Published June 1, 1976 | Version v1
Journal article

Discovery of a 283-second periodic variation in the X-ray source 3U 0900--40

  • 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

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