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The Redshift of Extragalactic Nebulae

Zwicky, Fritz (1933) The Redshift of Extragalactic Nebulae. Helvetica Physica Acta, 6 . pp. 110-127. ISSN 0018-0238. doi:10.5169/seals-110267. https://resolver.caltech.edu/CaltechAUTHORS:20190108-092708978

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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.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.5169/seals-110267DOIOriginal Article
https://arxiv.org/abs/1711.01693arXivDiscussion Paper
http://ned.ipac.caltech.edu/level5/March17/Zwicky/frames.htmlAuthorTranslated Article
Other Contributors:
ContributionOther Contributors NameIdentifierPersonID (may be blank)
TranslatorAndernach, HeinzAndernach-HUNSPECIFIED
Alternate Title:Die Rotverschiebung von extragalaktischen Nebeln
Additional Information:© 1933 Birkhaeuser. Translated by H. Andernach.
DOI:10.5169/seals-110267
Record Number:CaltechAUTHORS:20190108-092708978
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190108-092708978
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:92130
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:08 Jan 2019 21:08
Last Modified:16 Nov 2021 03:47

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