Are galaxy distributions scale invariant? A perspective from dynamical systems theory

DOI10.1016/S0378-4371(02)00615-5zbMath0995.85004arXivastro-ph/9703046OpenAlexW3099286596MaRDI QIDQ1598991

Joseph L. McCauley

Publication date: 4 June 2002

Published in: Physica A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/9703046

zbMATH Keywords

measure theorydimension spectrumcorrelation integral

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Dynamical systems in classical and celestial mechanics (37N05)

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