Fig. 2.
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MUSE data of NGC 4277. Left panel: MUSE reconstructed image with pseudo-slits (white lines) and a bar isophote (black ellipse). The FOV is 50 × 60 arcmin2 and the disc major axis is parallel to the vertical axis. Central panel: mean stellar LOS velocity map of NGC 4277 with a bar isophote (black ellipse). The FOV is 50 × 60 arcmin2 and the disc major axis is parallel to the vertical axis. Right panel: kinematic integrals ⟨V⟩ as a function of photometric integrals ⟨X⟩. The black solid line represents the best fit to the data.
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