An Apparent Gap in Stellar Mass Distributions around 0.7 Solar Masses and a Possible Explanation

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dc.creatorOldershaw, Robert L.
dc.date2000-11-26
dc.date2000-11-28
dc.date.accessioned2026-07-07T07:38:53Z
dc.date.available2026-07-07T07:38:53Z
dc.descriptionMass functions for samples of white dwarf stars and for a large heterogeneous sample of nearby stars appear to have unexplained deficits in the range of 0.70 to 0.75 Solar Masses. The existence, or non-existence, of this anomaly constitutes a definitive test of a fractal cosmological model that inherently predicts a gap in stellar mass functions at about 0.73 Solar Masses.
dc.description18 pages with 4 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0011480
dc.identifierhttp://arxiv.org/abs/astro-ph/0011480
dc.identifierAstrophys.Space Sci. 278 (2001) 425-432
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/121259
dc.subjectAstrophysics
dc.titleAn Apparent Gap in Stellar Mass Distributions around 0.7 Solar Masses and a Possible Explanation
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