Direct evidence of hierarchical assembly at low masses from isolated dwarf galaxy groups
Sabrina Stierwalt, Sandra E. Liss, Kelsey E. Johnson, David R. Patton,, George C. Privon, Gurtina Besla, Nitya Kallivayalil, Mary Putman

TL;DR
This paper presents direct observational evidence of hierarchical assembly in low-mass dwarf galaxy groups, supporting predictions of structure formation theories and providing insights into galaxy formation at small scales.
Contribution
It reports the discovery of seven isolated dwarf galaxy groups, offering rare empirical evidence of hierarchical assembly at low masses, consistent with Cold Dark Matter predictions.
Findings
Seven isolated dwarf galaxy groups identified with 3-5 members each
Groups have baryonic masses between 4.4 x 10^9 and 2 x 10^10 Msun
Mass-to-light ratios less than 100, indicating gravitational binding
Abstract
The demographics of dwarf galaxy populations have long been in tension with predictions from the Cold Dark Matter (CDM) paradigm. If primordial density fluctuations were scale-free as predicted, dwarf galaxies should themselves host dark matter subhaloes, the most massive of which may have undergone star formation resulting in dwarf galaxy groups. Ensembles of dwarf galaxies are observed as satellites of more massive galaxies, and there is observational and theoretical evidence to suggest that these satellites at z=0 were captured by the massive host halo as a group. However, the evolution of dwarf galaxies is highly susceptible to environment making these satellite groups imperfect probes of CDM in the low mass regime. We have identified one of the clearest examples to date of hierarchical structure formation at low masses: seven isolated, spectroscopically confirmed groups with only…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Cosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena
