Phenomenological analysis of observed relations for low-redshift galaxies
Maximum-likelihood estimates are made for the exponent p in the phenomenological redshift-distance relation z [unk] r(p) for galaxies at redshifts ≲0.03, on the basis of redshift (z)-magnitude (m)-apparent diameter (θ) observations given in the Reference Catalogue of Bright Galaxies [de Vaucouleurs,...
Guardat en:
| Publicat a: | Proc Natl Acad Sci U S A |
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| Autors principals: | , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
National Academy of Sciences
1975
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| Matèries: | |
| Accés en línia: | https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC388794/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/16592289/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.72.12.4691 |
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