No modulation of the 3-6 keV X-ray intensity of Sco X-1 at a level of excess of 1% was observed at the optical period of .787313d. Evidence is found for shot-noise character in a large fraction of the X-ray emission. Almost all of the Sco X-1 emission can be synthesized in terms of approximately 200 shots per day, each with a duration of approximately 1/3 day. A pinhole camera was used to obtain data and the data were statistically analyzed
Analysis of All-Sky Monitor observations of Cir X-1 (3U1516-56) over the period October 1975 - April...
A series of optical and X-ray observations of Sco X-1 and Cyg X-2 by UHURU satellite is reported. Re...
Sco X-1 is the brightest extrasolar X-ray source in the sky. Additional knowledge of its output in t...
Preliminary results from the Ariel-5 all-sky X-ray monitor are presented, along with sufficient expe...
Sco X-1 was monitored at optical and X-ray wavelengths from 1970 April 26 to 1970 May 21. The optica...
The optical flux of Seo X-1 was continuously monitored on five separate nights between April and Jun...
Since the optical identification of Sco X-1 by Sandage et al., a large number of photometric observa...
Data obtained during five nights of continuous monitoring of the X-ray source Seo X-1 between April ...
An attempt to observe the discrete X-ray source Sco X-1 on 20 September 1973 between 0856 and 0920 U...
No evidence for stable 2-10 keV periodic emission from Cas A or Tycho in the period range 1 msec to ...
X ray astronomy rocket experiment for identification and positioning of SCO X-1 strong X ray sourc
Sco X-1 has been the subject of many multiwavelength studies in the past, being the brightest persis...
We report the observation of sudden changes in the intensity of Sco X-1 by a factor of about three i...
The correlation between the X-ray and the optical emissions of Sco X-1 provides an important clue to...
The millisecond bursts from Cyg X-1 are investigated and the overall chaotic variability for the bul...
Analysis of All-Sky Monitor observations of Cir X-1 (3U1516-56) over the period October 1975 - April...
A series of optical and X-ray observations of Sco X-1 and Cyg X-2 by UHURU satellite is reported. Re...
Sco X-1 is the brightest extrasolar X-ray source in the sky. Additional knowledge of its output in t...
Preliminary results from the Ariel-5 all-sky X-ray monitor are presented, along with sufficient expe...
Sco X-1 was monitored at optical and X-ray wavelengths from 1970 April 26 to 1970 May 21. The optica...
The optical flux of Seo X-1 was continuously monitored on five separate nights between April and Jun...
Since the optical identification of Sco X-1 by Sandage et al., a large number of photometric observa...
Data obtained during five nights of continuous monitoring of the X-ray source Seo X-1 between April ...
An attempt to observe the discrete X-ray source Sco X-1 on 20 September 1973 between 0856 and 0920 U...
No evidence for stable 2-10 keV periodic emission from Cas A or Tycho in the period range 1 msec to ...
X ray astronomy rocket experiment for identification and positioning of SCO X-1 strong X ray sourc
Sco X-1 has been the subject of many multiwavelength studies in the past, being the brightest persis...
We report the observation of sudden changes in the intensity of Sco X-1 by a factor of about three i...
The correlation between the X-ray and the optical emissions of Sco X-1 provides an important clue to...
The millisecond bursts from Cyg X-1 are investigated and the overall chaotic variability for the bul...
Analysis of All-Sky Monitor observations of Cir X-1 (3U1516-56) over the period October 1975 - April...
A series of optical and X-ray observations of Sco X-1 and Cyg X-2 by UHURU satellite is reported. Re...
Sco X-1 is the brightest extrasolar X-ray source in the sky. Additional knowledge of its output in t...