Abstract
We have measured dielectronic recombination (DR) and electron impact ionization (EII) for a range of astrophysically relevant atomic ions (Fe9+, Fe10+, O3+, and Mg6+). The experiments were performed in a merged beams setup at the heavy-ion storage ring TSR in Heidelberg, Germany. Here we discuss the importance of our data for astrophysical modelling and compare our experimental results with the previously recommended data and with modern theoretical calculations. We have parameterized our data using simple fiting formulae for convenient inclusion into astrophysical modelling codes.
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.
