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October 5, 2025The Astrophysical Journal LettersOpen Access

Characterization of Two Cool Galaxy Outflow Candidates Using Mid-infrared Emission from Polycyclic Aromatic Hydrocarbons

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Authors

JSJessica SutterKSKarin SandströmRCRyan Chown

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Overview

Analysis reveals cool gas outflows in low-mass Virgo cluster galaxies, indicating new identification methods. Extended structures in mid-infrared emissions highlight possible physical processes involved.

Key Points

  • Two candidate cool galactic outflows were identified in low-mass Virgo cluster galaxies.
  • Enhanced mid-infrared observations revealed structures bright in the PAH-tracing bands.
  • This approach highlights the potential of mid-infrared methods for studying outflows in lower star-formation galaxies.
  • These findings suggest that our understanding of gas outflows in galaxy evolution can be improved through deeper infrared studies.

Cite This Study

Sutter et al. (2025) studied this question.

synapsesocial.com/papers/68e24e65d6d66a53c2473545https://doi.org/10.3847/2041-8213/ae08b7
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