Add to ORKGAriel-5 all sky monitor data on Cyg X-1 X-ray intensity increase during 1975 are analyzed. Data cover rise, maximum, and decay variability of the constellation. Special attention was given to the failure of the increase to decay over the specified period of 5.6 days
A search for a 78.4 day modulation in the high energy X-ray flux observed with OSO-8 and in the U-ba...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2001.Includes bibliographi...
The Ariel-V satellite monitored the X-ray light curve of A1524-62 almost continuously from 40 days p...
Observations of Cyg X-1 between October 1974 and July 1975 reveal a persistent 5.6 day modulation of...
The three bright 3-6 keV X-ray sources in Cygnus are examined for regular temporal variability with ...
Analysis of All-Sky Monitor observations of Cir X-1 (3U1516-56) over the period October 1975 - April...
Data taken from the Ariel-5 All Sky Monitor and the Ariel-5 Sky Survey Experiment are analyzed. It i...
A summary of results obtained from the first year of Ariel-5 all-sky monitor operation is presented....
The All-Sky Monitor on Ariel 5 has observed the Aquila-Serpens region on a quasi-continuous basis si...
Evidence for a persistent 11.17 + or - .10d period from Cyg X-2 is presented from one year of accumu...
X-rays from Cygnus X-3 were observed during early 1978 with the detectors of the SAS-3 satellite. Th...
High-energy X-ray spectra of the Crab Nebula, Cyg- XR-1, and Cen A were determined from observations...
Preliminary results from the Ariel-5 all-sky X-ray monitor are presented, along with sufficient expe...
The 1.7-40 keV spectra of Cyg X-3 obtained about a year apart, using the same rocket payload, show l...
X-ray sources are reported for HZ Herculis, supergiant primary X-ray binary systems, and Cyg X-3. Al...
A search for a 78.4 day modulation in the high energy X-ray flux observed with OSO-8 and in the U-ba...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2001.Includes bibliographi...
The Ariel-V satellite monitored the X-ray light curve of A1524-62 almost continuously from 40 days p...
Observations of Cyg X-1 between October 1974 and July 1975 reveal a persistent 5.6 day modulation of...
The three bright 3-6 keV X-ray sources in Cygnus are examined for regular temporal variability with ...
Analysis of All-Sky Monitor observations of Cir X-1 (3U1516-56) over the period October 1975 - April...
Data taken from the Ariel-5 All Sky Monitor and the Ariel-5 Sky Survey Experiment are analyzed. It i...
A summary of results obtained from the first year of Ariel-5 all-sky monitor operation is presented....
The All-Sky Monitor on Ariel 5 has observed the Aquila-Serpens region on a quasi-continuous basis si...
Evidence for a persistent 11.17 + or - .10d period from Cyg X-2 is presented from one year of accumu...
X-rays from Cygnus X-3 were observed during early 1978 with the detectors of the SAS-3 satellite. Th...
High-energy X-ray spectra of the Crab Nebula, Cyg- XR-1, and Cen A were determined from observations...
Preliminary results from the Ariel-5 all-sky X-ray monitor are presented, along with sufficient expe...
The 1.7-40 keV spectra of Cyg X-3 obtained about a year apart, using the same rocket payload, show l...
X-ray sources are reported for HZ Herculis, supergiant primary X-ray binary systems, and Cyg X-3. Al...
A search for a 78.4 day modulation in the high energy X-ray flux observed with OSO-8 and in the U-ba...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2001.Includes bibliographi...
The Ariel-V satellite monitored the X-ray light curve of A1524-62 almost continuously from 40 days p...