ON SOME PREDICTED AND OBSERVED FEATURES OF QUASI-STELLAR SOURCES,
Abstract
The purpose of this paper is to correlate or explain some observed features of quasi-stellar sources in a way that enables one to predict with simple models: (a) the relative strengths of the Lyman lines (np > ls transitions in hydrogen) that may be observed and (b) the optical depth of the nebulae beyond the Lyman continuum (hv > 13.6 eV).
Document Details
- Document Type
- Technical Report
- Publication Date
- Jan 01, 1966
- Accession Number
- AD0633013
Entities
People
- John N. Bahcall
Organizations
- California Institute of Technology