(1) DPh/EP/Ap, Section d'Astrophysique, Centre d'Etudes Nucleaires de Saclay, France;(2) Harvard/Smithsonian Center for Astrophysics, 02138 Cambridge, Massachusetts, USA
Abstract:
Conclusions The present results confirm the thermal nature of the interstellar soft X-ray emission and give rather clear evidence of the Oxygen and Carbon contribution.