CO emission is detected ~0.85 kpc above the disk of NGC 4565 at three positions, with a high-velocity component whose kinetic energy (~10^54 erg) is difficult to explain by stellar feedback alone, suggesting possible external inflow.
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A CO detection in the off-plane region of the edge-on galaxy NGC 4565 with the Nobeyama 45-m telescope
CO emission is detected ~0.85 kpc above the disk of NGC 4565 at three positions, with a high-velocity component whose kinetic energy (~10^54 erg) is difficult to explain by stellar feedback alone, suggesting possible external inflow.