On the possible connection between the amount of gas in galaxies, the activity of their nuclei and their belonging to a cluster

Details On the possible connection between the amount of gas in galaxies, the activity of their nuclei and their belonging to a cluster On the possible connection between the amount of gas in galaxies, the activity of their nuclei and their belonging to a cluster

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976stin...7710985k&link_type=abstract

On the possible connection between the amount of gas in galaxies, the activity of their nuclei and their belonging to a cluster

Computer Science

Galactic Clusters, Galactic Nuclei, Gas Density, Gas Spectroscopy, Gaseous Self-Diffusion, Hydrogen Compounds, Iodides, Radio Galaxies, Star Formation Rate

Scientific paper

Optical and radio wavelength data available on fast S- and E-galaxies in regular clusters were analyzed. These galaxies are deficient in gas, have slower star formation rates and less active nuclei when compared to similar field galaxies. The slow massive galaxies in central regions of rich clusters, on the contrary, contain more gas and have more active nuclei.

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