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AbstractWe study the radial acceleration relation (RAR) for early type galaxies (ETGs) in the SDSS MaNGA MPL5 data set. The complete ETG sample show a slightly offset RAR from the relation reported by McGaugh et al. (2016) at the low acceleration end; we find that the deviation is due to the fact that the slow rotators show a systematically higher acceleration relation than the McGaugh's RAR, while the fast rotators show a consistent acceleration relation to McGaugh's RAR.

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Edited by cheritys123 on Jul 24, 2020 01:05:26
Edited by cheritys123 on Jul 24, 2020 01:05:13

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