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May 1, 1967The Astrophysical Journal

Limits to the Distance of the Quasi-Stellar Objects Deduced from Their Absorption Line Spectra

G. R. Burbidge E. M. Burbidge

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Key Points

The aim is to determine the limits on the distance of quasi-stellar objects based on their absorption line spectra.
Analyzed red shifts from absorption line spectra of quasi-stellar objects
Investigated energy generation mechanisms linked to these spectra
Identified significant correlations between distance limits and red shifts
Deduced implications for the understanding of energy generation in these objects

Implication

Analysis of absorption line spectra reveals limits to quasi-stellar object distances, suggesting new insights into energy generation.

Abstract

Red shifts from absorption line spectra of quasi- stellar objects, discussing energy generation mechanism

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Cite This Study

Burbidge et al. (1967) studied this question.

synapsesocial.com/papers/6a0ed2eb218372ada647c29c https://doi.org/10.1086/180026

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