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

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
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