Born to be Starless: Revisiting the Missing Satellite Problem
Seyoung Jeon, Sukyoung K. Yi, Emanuele Contini, Yohan Dubois, San Han, Katarina Kraljic, Sebastien Peirani, Christophe Pichon, Jinsu Rhee

TL;DR
This study uses high-resolution cosmological simulations to show that most subhalos around Milky Way-like galaxies are starless because they are born in regions with insufficient gas density for star formation, primarily due to reionization effects.
Contribution
It demonstrates that starless subhalos are born without stars due to reionization, challenging previous ideas that they become starless through feedback or environmental effects.
Findings
Most subhalos are starless due to initial conditions.
Reionization prevents gas cooling in low-density regions.
Number of satellites aligns with observations.
Abstract
The massive Local Group galaxies both host substantially fewer satellites than the subhalos expected from the cold dark matter paradigm, and the recent investigations have highlighted the interplay between baryons and dark matter. We investigate the processes that make subhalos starless, using high-resolution cosmological simulations. We found that the number of satellites around Milky Way analogs closely aligns with observations, which accords with recent studies. In our simulations, the majority of subhalos are devoid of stars, i.e., "starless." We first examined supernova feedback and the environmental effects associated with subhalos' orbital motion as candidates of origin. However, neither seems to be the main driver. Supernova feedback causes a reduction of cold gas in "starred" subhalos, but its impact is not significant. In the case of starless subhalos, supernova feedback is…
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