activity
19932026
most citedModified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions

895 citations · 15.5k across the 178 of their papers we have counts for

collaborators
Showing 2014 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2014★ 44 cited

The Third Law of Galactic Rotation

Stacy S. McGaugh

I review the connection between dynamics and the baryonic mass distribution in rotationally supported galaxies. The enclosed dynamical mass-to-light ratio increases with decreasing…

astro-ph.GA2014★ 62 cited

Stellar Populations and the Star Formation Histories of LSB Galaxies: III. Stellar Population Models

James Schombert, Stacy McGaugh

A series of population models are designed to explore the star formation history of gas-rich, low surface brightness (LSB) galaxies. LSB galaxies are unique in having properties of…

astro-ph.GA2014★ 243 cited

Color--Mass-to-Light Ratio Relations for Disk Galaxies

Stacy McGaugh, Jim Schombert

We combine Spitzer observations of a sample of disk galaxies spanning over 10 magnitudes in luminosity with optical luminosities and colors to test population synthesis pres…

astro-ph.GA2014★ 39 cited

Co-orbiting planes of sub-halos are similarly unlikely around paired and isolated hosts

Marcel S. Pawlowski, Stacy S. McGaugh

Sub-halos in dark-matter-based cosmological simulations tend to be distributed approximately isotropically around their host. The existence of highly flattened, co-orbiting planes…

astro-ph.GA2014★ 55 cited

Perseus I and the NGC 3109 association in the context of the Local Group dwarf galaxy structures

Marcel S. Pawlowski, Stacy S. McGaugh

The recently discovered dwarf galaxy Perseus I appears to be associated with the dominant plane of non-satellite galaxies in the Local Group (LG). We predict its velocity dispersio…

astro-ph.GA2014★ 6 cited

The Inner Dynamical Mass Across Galaxy Morphology: A Weak Scaling with Total Stellar Mass

Rachel Kuzio de Naray, Stacy S. McGaugh

We compile a sample of dispersion-supported and rotation-supported galaxies for which the dynamical mass enclosed at 500 pc can be measured. We find that this dynamical quantity in…