The paucity of globular clusters around the field elliptical NGC 7507
J. P. Caso (1), T. Richtler (2), L. P. Bassino (1), R. Salinas (3), R., R. Lane (2), A. Romanowsky (4) ((1) Facultad de Ciencias Astron\'omicas y, Geof\'isicas de la Universidad Nacional de La Plata, Consejo Nacional de, Investigaciones Cient\'ificas y T\'ecnicas

TL;DR
This study reveals that the isolated elliptical galaxy NGC 7507 has an exceptionally poor globular cluster system, highlighting the influence of environment on globular cluster formation and richness.
Contribution
It provides the first detailed analysis of the globular cluster system of NGC 7507, showing its low richness and subpopulation characteristics, emphasizing environmental effects.
Findings
GCS richness is very low with S_N ~ 0.6.
Identified three globular cluster subpopulations with distinct colours.
The galaxy's GCS is poor despite its mass, illustrating environmental impact.
Abstract
Context: There is strong evidence that globular cluster systems (GCSs) of massive galaxies are largely assembled by infall/accretion processes. Therefore, we expect the GCSs of isolated elliptical galaxies to be poor. Alhough not completely isolated, NGC 7507 is a massive field elliptical galaxy with an apparently very low dark matter content. Aims: We determine the richness, the colour distribution, and the structural properties of the GCS of NGC 7507. Methods: We perform wide-field Washington photometry with data obtained with the MOSAIC II camera at the 4m-Blanco telescope, CTIO. Results: The GCS is very poor with S_N ~ 0.6. We identify three subpopulations with peaks at (C-T1) colours of 1.21, 1.42, and 1.72. The bluest population may represent the old, metal-poor component. This interpretation is supported by its shallow density profile. The red population is more concentrated,…
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