A new hypothesis to account for the red-shift in the spectra of distant stars
- DOI
- 10.1016/0031-9163(64)90462-7
- Published
- 1964-12
- Container
- Physics Letters
- Publisher
- Elsevier BV
- Open access
- unknown
Credibility signals
uncertain Score 64/100 under policy 1.0.0. This is a metadata assessment, not a judgment of the paper's conclusions.
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Cite this work
BibTeX
@article{allodium:10.1016/0031-9163-64-90462-7,
title = {A new hypothesis to account for the red-shift in the spectra of distant stars},
author = {R. Fürth},
year = {1964},
journal = {Physics Letters},
doi = {10.1016/0031-9163(64)90462-7},
url = {https://doi.org/10.1016/0031-9163(64)90462-7}
}RIS
TY - JOUR TI - A new hypothesis to account for the red-shift in the spectra of distant stars AU - R. Fürth PY - 1964 JO - Physics Letters DO - 10.1016/0031-9163(64)90462-7 UR - https://doi.org/10.1016/0031-9163(64)90462-7 ER -
APA
Fürth, R. (1964). A new hypothesis to account for the red-shift in the spectra of distant stars. Physics Letters. https://doi.org/10.1016/0031-9163(64)90462-7
Source records
- crossref · retrieved 2026-09-26T23:58:19.576Z