Published 1976 | Version v1
Report

Intensity and spectral variations of Cyg X-1 observed from balloons

  • 1. Univ. of California, San Diego, La Jolla

Description

Observations of Cyg X-1 with a 20 to 200 keV balloon carried x-ray telescope in 1969, 1970, and 1972 are presented. These results reveal the following characteristics of Cyg X-1: The steep spectrum observed at E less than 10 keV during the ''radio quiet'' phase can extend to 200 keV. This phase may have lasted 21 months (July 1969 to March 1971). The flux at 30 keV can vary from 1.1 x 10-2 to 1.4 x 10-3 ph (cm2-sec-keV)-1 and that at 100 keV from 1.4 x 10-3 to 10-4. The low flux values are factors of 3 and 8 below the ''normal'' values at 30 and 100 keV respectively, are rarely observed, and may be associated with the early phase of the 1971 April x-ray transition. During some one hour periods the intensity remained constant to approximately 20% and during other periods it varied a factor 2 in 5 minutes and a factor 10 in 1 hour. Complex spectral variations accompanied the intensity changes

Additional details

Publishing Information

Imprint Title
X-ray binaries
Journal Page Range
p. 407-424.
Report number
CONF-7510169--

Conference

Title
Symposium on x-ray binaries.
Dates
20 - 22 Oct 1975.
Place
Greenbelt, Maryland, United States of America (USA).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
9364375
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COSMIC X-RAY SOURCES; RADIATION FLUX; VARIATIONS; X-RAY SPECTRA
Descriptors DEC
COSMIC RAY SOURCES; SPECTRA