Analytical properties of the R^(1/m) luminosity law
arXiv:astro-ph/9911078
Abstract
In this paper we describe some analytical properties of the R^{1/m} law proposed by Sersic (1968) to categorize the photometric profiles of elliptical galaxies. In particular, we present the full asymptotic expansion for the dimensionless scale factor b(m) that is introduced when referring the profile to the standard effective radius. Surprisingly, our asymptotic analysis turns out to be useful even for values of m as low as unity, thus providing a unified analytical tool for observational and theoretical investigations based on the R^{1/m} law for the entire range of interesting photometric profiles, from spiral to elliptical galaxies.
9 pages, 1 figure, to be published in A&A (main journal)
Cited by in corpus (16)
- SKIRT: an Advanced Dust Radiative Transfer Code with a User-Friendly Architecture
- Full spectrum fitting with photometry in pPXF: stellar population versus dynamical masses, non-parametric star formation history and metallicity for 3200 LEGA-C galaxies at redshift z~0.8
- EPOCHS VI: The Size and Shape Evolution of Galaxies since z ~ 8 with JWST Observations
- Scrutinizing FR 0 Radio Galaxies as Ultra-High-Energy Cosmic Ray Source Candidates
- The dawn of disks: unveiling the turbulent ionised gas kinematics of the galaxy population at with JWST/NIRCam grism spectroscopy
- One never walks alone: the effect of the perturber population on subhalo measurements in strong gravitational lenses
- An elusive dark central mass in the globular cluster M4
- Detection of the 2175Å UV Bump at z>7: Evidence for Rapid Dust Evolution in a Merging Reionisation-Era Galaxy
- When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
- WISDOM Project -- XIX. Figures of merit for supermassive black hole mass measurements using molecular gas and/or megamaser kinematics
- Pixel-level modelling of group-scale strong lens CASSOWARY 19
- Testing the Surface Brightness Fluctuation Method on Dwarf Galaxies in the COSMOS Field
- Impact of Dynamical Friction on the Tidal Formation of NGC 1052-DF2
- The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
- Time delay measurements with Broken Power Law model
- Imprints of tidal interactions on the stellar distribution of satellite galaxies: implications for dark matter deficient galaxies