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Figure 1:
Solid line: Effelsberg 100-m spectrum of the central position.
Dashed line: spectrum of the VLA data. Dotted line: 3![]() ![]() |
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Figure 2:
Solid lines: Effelsberg 100-m spectra of the four off-center positions.
Their locations with respect to the galaxy center are marked on top of each panel.
Dashed line: synthesized VLA spectra which only show H I disk emission.
Dotted line: 3![]() |
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Figure 3:
Evolution of the model stellar and gas disk.
The disk is seen face-on and rotates counter-clockwise. The arrow
indicates the direction of ram pressure, i.e. it is opposite to
the galaxy's velocity vector. The size of the arrow is proportional
to
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Figure 4:
Evolution of the model stellar and gas disk.
The position and inclination angle of NGC 4388 (
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Figure 5: ISM radial velocity as a function of the projected distance to the galaxy center. |
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Figure 6:
Left panel: stellar distribution as contours, gas distribution as greyscales.
Only gas with a local density greater than ![]() |
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Figure 7: Left panel: model 100-m spectrum at the central (C) position. Right panel: model 100-m spectrum at the northeastern (NE) position. Velocities are given relative to the systemic velocity of NGC 4388. |
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