Abstract
ABSTRACT A temperature correction for the Corliss and Bozman arc has been determined from a comparison of their oscillator strengths for Fe I with recent laboratory measurements and the resulting excitation-dependent adjustment applied to the oscillator strengths of 58 lines of Zr ii and two of Sr I. The absolute scales of these oscillator strengths are then established by line strengths in the solar spectrum assuming the solar abundances of these elements to be those of the chondritic meteorites. Key words: oscillator strengths - zirconium - solar abundances
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 callMore From: Publications of the Astronomical Society of the Pacific
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.
