Evidence for gas around two radio galaxies at the Coma cluster periphery

Details Evidence for gas around two radio galaxies at the Coma cluster periphery Evidence for gas around two radio galaxies at the Coma cluster periphery

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...213...49v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 213, no. 1-2, April 1989, p. 49-60.

Astronomy and Astrophysics

Astrophysics

11

Cosmic Gases, Galactic Clusters, Galactic Structure, Intergalactic Media, Radio Galaxies, Elliptical Galaxies, Very Large Array (Vla)

Scientific paper

Multifrequency high-resolution high-sensitivity observations were obtained for two radio galaxies at the Coma cluster periphery, NGC 4789 and NGC 4827. NGC 4789 displays a twin tail structure and NGC 4827 has a Z-shaped morphology. A model for NGC 4789 is presented which considers the effect of external ram pressure due to the galaxy motion. The results suggest that the gas around these two radio galaxies is denser than expected for this cluster region.

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