Abstract
The possibility of detectable extragalactic radio recombination lines is explored. Stimulated recombination lines may be detectable from the nuclei of active galaxies and quasars at the mJy level. The major uncertainty concerns the geometry of the nuclear emission-line region - its size and homogeneity. Low-frequency recombination lines may also be detectable from optical absorption-line regions in the directions of distant radio sources.
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.
