Abstract
Using the photometric data from the Next Generation Fornax Survey, we find a significant radial alignment signal among the Fornax dwarf galaxies. For the first time, we report that the radial alignment signal of nucleated dwarfs is stronger than that of non-nucleated ones at the 2.4 σ confidence level, and the dwarfs located in the outer region ( R > R vir /3; R vir is the Fornax virial radius) show a slightly stronger radial alignment signal than those in the inner region ( R
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CITATION STYLE
Rong, Y., Puzia, T. H., Eigenthaler, P., Ordenes-Briceño, Y., Taylor, M. A., Muñoz, R. P., … Johnston, E. J. (2019). The Next Generation Fornax Survey (NGFS). VI. The Alignment of Dwarf Galaxies in the Fornax Cluster. The Astrophysical Journal, 883(1), 56. https://doi.org/10.3847/1538-4357/ab3725
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