Add to ORKGEvidence for a persistent 11.17 + or - .10d period from Cyg X-2 is presented from one year of accumulated data from the Ariel-5 all-sky monitor. The effect is not a simple sidereal alias of a true source period close to one day
Twelve hundred days of 3-6 keV X-ray data from Her X-1, Vela X-1 and Cen X-3 accumulated with the Ar...
The X-ray spectra from three observations of the X-ray binary Cyg X-3 by the cosmic X-ray spectrosco...
We present X-ray and infrared observations of the X-ray source CXOGC J174536.1-285638. Previous obse...
Data taken from the Ariel-5 All Sky Monitor and the Ariel-5 Sky Survey Experiment are analyzed. It i...
The three bright 3-6 keV X-ray sources in Cygnus are examined for regular temporal variability with ...
Ariel-5 all sky monitor data on Cyg X-1 X-ray intensity increase during 1975 are analyzed. Data cove...
Observations of Cyg X-1 between October 1974 and July 1975 reveal a persistent 5.6 day modulation of...
Analysis of All-Sky Monitor observations of Cir X-1 (3U1516-56) over the period October 1975 - April...
Preliminary results from the Ariel-5 all-sky X-ray monitor are presented, along with sufficient expe...
X-rays from Cygnus X-3 were observed during early 1978 with the detectors of the SAS-3 satellite. Th...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2001.Includes bibliographi...
The OAO-3 satellite was used for several months' observation of the loss mass X-ray binary sources 2...
A summary of results obtained from the first year of Ariel-5 all-sky monitor operation is presented....
We present a detailed period analysis of the bright Cepheid-type variable star V1154 Cygni (V1154 C...
Using data obtained with the Rossi X-ray Timing Explorer, we report the detection of a 5 Hz quasi-pe...
Twelve hundred days of 3-6 keV X-ray data from Her X-1, Vela X-1 and Cen X-3 accumulated with the Ar...
The X-ray spectra from three observations of the X-ray binary Cyg X-3 by the cosmic X-ray spectrosco...
We present X-ray and infrared observations of the X-ray source CXOGC J174536.1-285638. Previous obse...
Data taken from the Ariel-5 All Sky Monitor and the Ariel-5 Sky Survey Experiment are analyzed. It i...
The three bright 3-6 keV X-ray sources in Cygnus are examined for regular temporal variability with ...
Ariel-5 all sky monitor data on Cyg X-1 X-ray intensity increase during 1975 are analyzed. Data cove...
Observations of Cyg X-1 between October 1974 and July 1975 reveal a persistent 5.6 day modulation of...
Analysis of All-Sky Monitor observations of Cir X-1 (3U1516-56) over the period October 1975 - April...
Preliminary results from the Ariel-5 all-sky X-ray monitor are presented, along with sufficient expe...
X-rays from Cygnus X-3 were observed during early 1978 with the detectors of the SAS-3 satellite. Th...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2001.Includes bibliographi...
The OAO-3 satellite was used for several months' observation of the loss mass X-ray binary sources 2...
A summary of results obtained from the first year of Ariel-5 all-sky monitor operation is presented....
We present a detailed period analysis of the bright Cepheid-type variable star V1154 Cygni (V1154 C...
Using data obtained with the Rossi X-ray Timing Explorer, we report the detection of a 5 Hz quasi-pe...
Twelve hundred days of 3-6 keV X-ray data from Her X-1, Vela X-1 and Cen X-3 accumulated with the Ar...
The X-ray spectra from three observations of the X-ray binary Cyg X-3 by the cosmic X-ray spectrosco...
We present X-ray and infrared observations of the X-ray source CXOGC J174536.1-285638. Previous obse...