Neutral Hydrogen content of dwarf galaxies in different environments
Hui-Jie Hu, Qi Guo, Pablo Renard, Hang Yang, Zheng Zheng, Yingjie, Jing, Hao Chen, and Hui Li

TL;DR
This study investigates how environment influences the neutral hydrogen content in dwarf galaxies by combining deep FAST observations with existing surveys, revealing environmental effects on gas content and galaxy evolution.
Contribution
It introduces a method of using deep FAST observations to study low HI content dwarf galaxies across environments, improving understanding of gas stripping processes.
Findings
Positive correlation between HI mass and stellar mass in dwarfs
Decreased HI-to-stellar mass ratio with increasing environment density
Steeper gas-stripping slope observed compared to simulations
Abstract
Environments play an important role in galaxy formation and evolution, particularly in regulating the content of neutral gas. However, current HI surveys have limitations in their depth, which prevents them from adequately studying low HI content galaxies in high-density regions. In this study, we address this issue by employing the Five-hundred-meter Aperture Spherical radio Telescope (FAST) with extensive integration times to complement the relatively shallow Arecibo Legacy Fast Arecibo L-band Feed Array (ALFALFA) HI survey. This approach allows us to explore the gas content of dwarf galaxies across various environments. We observe a positive relationship between HI mass and stellar mass in dwarf galaxies, with a well-defined upper boundary for HI mass that holds true in both observations and simulations. Furthermore, we find a decrease in the HI-to-stellar mass ratio ($\rm M_{\rm…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Galaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research
