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The Morphological Luminosity Function
1988We obtain the morphological luminosity function for galaxies assuming that they form at high density regions of a filtered Gaussian random field. We compare our results with some observations of the LF for E and E+SO galaxies. Using scale-free spectra, we obtain bell-shaped curves that follow the observations.
J. L. Sanz, E. Martínez-González
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The stellar luminosity function
2000The stellar luminosity function, Φ(M) — the number of stars per unit absolute magnitude per unit volume is one of the fundamental quantities required for understanding star formation and investigating the structure of our Galaxy. In recent years, most emphasis has been placed on determining the shape of Φ(M) at faint magnitude — and hence the mass ...
I. Neill Reid, Suzanne L. Hawley
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Luminosity Functions and the Mass Function
1995The determination of the Mass Function (MF) at the bottom of the Main Sequence is subject to severe uncertainties, due both to the very low intrinsic luminosity of these stars and to their rapidly varying Mass-Luminosity (ML) relation. A potentially very important field of exploration, although its present results are still to be correctly examined and
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The Cluster Galaxy Luminosity Function
Astrophysics and Space Science, 1999Our project to assess the LF of galaxies in clusters is giving the first results. A universal LF shape cannot be supported and the evolution has to be taken into account to explain differences. The blue galaxy distribution is also investigated.
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Female erectile tissues and sexual dysfunction after pelvic radiotherapy: A scoping review
Ca-A Cancer Journal for Clinicians, 2022Deborah C Marshall +2 more
exaly
Luminosity function of stars [PDF]
Astrophysics, 1977 R. A. Bartaya, E. K. Kharadze
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A systematic review of rehabilitation and exercise recommendations in oncology guidelines
Ca-A Cancer Journal for Clinicians, 2021Kathleen Doyle Lyons +2 more
exaly
The Quasar Luminosity Function
1993Recent work on the quasar luminosity function at radio, optical and X-ray wavelengths is reviewed. It is demonstrated that the evolution of the quasar luminosity function in all three regimes is marked by a strong and approximately similar power-law increase in luminosity, L ∝ (1 + z) 3±0.5, between the present epoch and z ≈ 2.
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