Fig. 7.
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Relation between the total specific angular momentum (Eq. (9)) and the number of satellites for SAGA galaxies, for which HI line measurements exist in the EDD database: gray circles with error bars denote the number of satellites detected up to the SAGA limit (Mr, 0 < −12.3); red crosses give the expected number of satellites if the relation from Javanmardi et al. (2019) holds.
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