Abstract
Hard X-ray observations using balloon borne instruments are quite competitive on the basis of sesitivity comparison. This paper describes spectral results of some of the binary X-ray sources obtained by using a scintillation counter telescope having a 3σ sensitivity of ∼10—6 cm—2s—1 keV—1 for 3 hour observation.
Published Version
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.