Abstract
The asymmetric distribution of galaxy redshifts in some nearby-group samples is explained as due to the existence of intragroup dust. The existence of a correlation between color excess of galaxies and radial velocity supports the hypothesis made.
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© 1990 Kluwer Academic Publishers
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Girardi, M., Giuricin, G., Mardirossian, F., Mezzetti, M. (1990). Possible Existence of Dust in Nearby Galaxy Group. In: Bussoletti, E., Vittone, A.A. (eds) Dusty Objects in the Universe. Astrophysics and Space Science Library, vol 165. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0661-7_35
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DOI: https://doi.org/10.1007/978-94-009-0661-7_35
Publisher Name: Springer, Dordrecht
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