Star Formation and Gas Reservoirs in Groups and Clusters

Star Formation and Gas Reservoirs in Groups and Clusters Star Formation and Gas Reservoirs in Groups and Clusters
  • Contact

    Rebecca Koopmann
    Department of Physics and Astronomy Union College Schenectady
    phone: 518-388-6786
    fax: 518-388-6947

  • Working language

    English

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Conference
United States
Schenectady, NY

Nearby groups and clusters provide laboratories to study the impact of environment on the properties of member galaxies, including gas content, star formation rates, morphology, and nuclear activity. This meeting will focus on the observed gas content and star formation properties of galaxies in groups and clusters in the local universe, and the current theoretical understanding of the dominant physical mechanisms at work.

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