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SPectral Observation of the Soft X-Ray Background and of the North Polar Spur with Solid State Spectrometers

Published online by Cambridge University Press:  04 August 2017

R. Rocchia
Affiliation:
Section d'Astrophysique, Centre d'Etudes Nucléaires de Saclay, France
M. Arnaud
Affiliation:
Section d'Astrophysique, Centre d'Etudes Nucléaires de Saclay, France
C. Blondel
Affiliation:
Section d'Astrophysique, Centre d'Etudes Nucléaires de Saclay, France
C. Cheron
Affiliation:
Section d'Astrophysique, Centre d'Etudes Nucléaires de Saclay, France
J. C. Christy
Affiliation:
Section d'Astrophysique, Centre d'Etudes Nucléaires de Saclay, France
L. Koch
Affiliation:
Section d'Astrophysique, Centre d'Etudes Nucléaires de Saclay, France
R. Rothenflug
Affiliation:
Section d'Astrophysique, Centre d'Etudes Nucléaires de Saclay, France
H. W. Schnopper
Affiliation:
Harvard/Smithsonian Center for Astrophysics, Cambridge, Massachusetts, USA
J. P. Delvaille
Affiliation:
Harvard/Smithsonian Center for Astrophysics, Cambridge, Massachusetts, USA

Extract

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In this paper, we present preliminary results of soft X-ray diffuse background observations. We observed two particular regions of the sky in the 0.3–1.5 keV range. The detection system consisted of three independent, 1 cm diameter, cooled solid state detectors. Nearly overlapping fields of view subtended a solid angle of approximately 1/4 sr. Except for the field of view, the whole set was similar to that described in Schnopper et al. (1982) (hereafter referred to as paper 1). This system was flown on board a three-axis stalibized rocket. The flight took place at White Sands Missile Range on 1981 May 4 at 0755 UT.

Type
IV. Old Supernova Remnants - Heating of the Interstellar Medium
Copyright
Copyright © Reidel 1983 

References

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