Abstract
The surroundings of 75 active SB galaxies are investigated. It is shown with a fairly high degree of certainty that more galaxies are observed in the direction of the bar than in other directions. It is concluded that this may be a consequence of the galaxy-forming activity of these galaxies. It is noted that the influence of the surroundings on a galaxy is traditionally discussed, although there is much evidence that the surroundings of a galaxy are shaped due to its activity.
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Harutyunian, H.A., Kalloghlian, A.T. Distribution of Galaxies with Respect to the Directions of the Bars of SB Galaxies. Astrophysics 45, 465–469 (2002). https://doi.org/10.1023/A:1021807129651
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DOI: https://doi.org/10.1023/A:1021807129651