Results 111 to 120 of about 254,332 (222)
openaire +3 more sources
The NRL OSO-4 Bragg crystal spectrometer instrument [PDF]
Two Bragg crystal spectrometers were placed on the OSO-4 satellite to study solar flare plasmas by their spectral emissions. The solar flare plasma parameters were measured with these spectrometers, which together covered a total wavelength range of 0.6 ...
Meekins, J. F.
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A search for X-ray polarization in cosmic X-ray sources [PDF]
Fifteen strong X-ray sources were observed by the X-ray polarimeters on board the OSO-8 satellite from 1975 to 1978. The final results of this search for X-ray polarization in cosmic sources are presented in the form of upper limits for the ten sources ...
Hughes, J. P., Long, K. S., Novick, R.
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Destinataire : Cárdenas Antognazzi, Silvina / Cárdenas Antognazzi, Mariela / Cárdenas Antognazzi ...
Irma, Antognazzi, Antognazzi, Irma
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Continuing data analysis of the AS/E grazing incidence X-ray telescope experiment on the OSO-4 satellite [PDF]
The work to correct and extend the calculation of the theoretical solar X-ray spectrum produced during earlier OSO-4 data analysis is reported along with the work to formulate models of active regions, and compare these models with the experimental ...
Haggerty, R. +6 more
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The 78.4 day period of Cygnus XR-1 [PDF]
A search for a 78.4 day modulation in the high energy X-ray flux observed with OSO-8 and in the U-band optical polarization is reported. It is suggested that if such a modulation does exist, it is more likely to be related to the rotation of the free ...
Caraveo, P. +6 more
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Este texto fue producido en el marco del Programa de Estudios Independientes del MACBA, Barcelona, y fue dedicado a la memoria del Profesor Oscar Terán (Buenos Aires, 1938-2008). A fin de ser aceptado en la presente revista, he tenido que realizar una serie de correcciones formales para ajustarlo a “La Academia”.
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Spectral variability in the X-ray pulsar GX 1+4 [PDF]
Observations of the galactic center region, hard X-ray source GX 1+4 by the GSFC X-ray spectroscopy experiment on OSO-8 confirm that GX 1+4 is a slow X-ray pulsar.
Becker, R. H. +6 more
core +1 more source
The article analyzes the results of the process components (PC) of technological plan (program) of official statistical observations (TP OSO) in Ukraine for 2014–2015.
Т. I. Lumpova, О. E. Ostapchuk
doaj

