Sco X-1 was monitored at optical and X-ray wavelengths from 1970 April 26 to 1970 May 21. The optical observations were made at six observatories around the world and the X-ray observations were made by the Vela satellites. There was a tendency for the object to show greater variability in X-ray when the object is optically bright. A discussion of the intensity histograms is presented for both the optical and X-ray observations. No evidence for optical or X-ray periodicity was detected
An attempt to observe the discrete X-ray source Sco X-1 on 20 September 1973 between 0856 and 0920 U...
We observed the low-mass X-ray binary Sco X-1 for 12 nights simultaneously using the Rossi X-Ray Tim...
The Goddard Space Flight Center Cosmic X-Ray Experiment aboard OSO-8 viewed the X-ray binary pulsar,...
A series of optical and X-ray observations of Sco X-1 and Cyg X-2 by UHURU satellite is reported. Re...
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 ...
The optical flux of Seo X-1 was continuously monitored on five separate nights between April and Jun...
No modulation of the 3-6 keV X-ray intensity of Sco X-1 at a level of excess of 1% was observed at t...
The correlation between the X-ray and the optical emissions of Sco X-1 provides an important clue 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...
Simultaneous hard X-ray and optical observations of Sco X-1 were carried out on 1971 May 1 at Hydera...
Results of rocket observations of SCO X-1 over the spectral range of 2∼20 keV are presented. ...
Sco X-1 is the brightest extrasolar X-ray source in the sky. Additional knowledge of its output in t...
We report the observation of sudden changes in the intensity of Sco X-1 by a factor of about three i...
An attempt to observe the discrete X-ray source Sco X-1 on 20 September 1973 between 0856 and 0920 U...
We observed the low-mass X-ray binary Sco X-1 for 12 nights simultaneously using the Rossi X-Ray Tim...
The Goddard Space Flight Center Cosmic X-Ray Experiment aboard OSO-8 viewed the X-ray binary pulsar,...
A series of optical and X-ray observations of Sco X-1 and Cyg X-2 by UHURU satellite is reported. Re...
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 ...
The optical flux of Seo X-1 was continuously monitored on five separate nights between April and Jun...
No modulation of the 3-6 keV X-ray intensity of Sco X-1 at a level of excess of 1% was observed at t...
The correlation between the X-ray and the optical emissions of Sco X-1 provides an important clue 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...
Simultaneous hard X-ray and optical observations of Sco X-1 were carried out on 1971 May 1 at Hydera...
Results of rocket observations of SCO X-1 over the spectral range of 2∼20 keV are presented. ...
Sco X-1 is the brightest extrasolar X-ray source in the sky. Additional knowledge of its output in t...
We report the observation of sudden changes in the intensity of Sco X-1 by a factor of about three i...
An attempt to observe the discrete X-ray source Sco X-1 on 20 September 1973 between 0856 and 0920 U...
We observed the low-mass X-ray binary Sco X-1 for 12 nights simultaneously using the Rossi X-Ray Tim...
The Goddard Space Flight Center Cosmic X-Ray Experiment aboard OSO-8 viewed the X-ray binary pulsar,...