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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,...

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Detalles Bibliográficos
Publicado en:Proc Natl Acad Sci U S A
Principais autores: Nicoll, J. F., Segal, I. E.
Formato: Artigo
Idioma:Inglês
Publicado: National Academy of Sciences 1975
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Acceso en liña: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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