Published 1933
| Version Reprint
Journal Article
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The Redshift of Extragalactic Nebulae
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Abstract
This gives a description of the most essential characteristics of extragalactic nebulae, as well as of the methods used to investigate these. In particular, the so-called redshift of extragalactic nebulae is discussed in detail. Various theories which have been proposed to explain this important phenomenon, are briefly discussed. Finally, it will be indicated to what extent the redshift promises to become of importance for the study of cosmic rays.
Additional Information
© 1933 Birkhaeuser. Translated by H. Andernach.Attached Files
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Fritz_redshift_of_extragalactic_nebulae.pdf
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Additional details
Additional titles
- Alternative title
- Die Rotverschiebung von extragalaktischen Nebeln
Identifiers
- Eprint ID
- 92130
- DOI
- 10.5169/seals-110267
- Resolver ID
- CaltechAUTHORS:20190108-092708978
Related works
- Describes
- 10.5169/seals-110267 (DOI)
- https://arxiv.org/abs/1711.01693 (URL)
- http://ned.ipac.caltech.edu/level5/March17/Zwicky/frames.html (URL)
Dates
- Created
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2019-01-08Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field