Superthin galaxies show higher stellar specific angular momentum j_s and larger exponential scale lengths R_D than ordinary bulgeless disks at given V_rot or M_s, with median spin parameter λ = 0.13 ± 0.01, an order of magnitude above comparison samples.
N., Banerjee, A., Chengalur, J.N
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The specific angular momenta of superthin galaxies: Cue to their origin?
Superthin galaxies show higher stellar specific angular momentum j_s and larger exponential scale lengths R_D than ordinary bulgeless disks at given V_rot or M_s, with median spin parameter λ = 0.13 ± 0.01, an order of magnitude above comparison samples.