Abstract
Gamma-ray line emission is calculated for thermonuclear excitation of very high-temperature (10/sup 10/--10/sup 12/ K) ions which may exist in accreting matter around neutron stars and black holes. The 4.438 MeV line from /sup 12/C* de-excitation should be the easiest to observe in both the continuous and transient emission spectra of such sources.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: 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.
