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arXiv · 1406.7625

Rotation Curve Anomaly and Galactic Warp in M51

Shouta Oikawa·Yoshiaki Sofue
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Abstract

We revisit the anomaly of rotation curve in the nearly face-on galaxy M51 that shows an apparently faster decrease of rotation velocity than the Keplerian law in the outer disk, further showing apparent counter rotation in the outermost HI disk. We interpret this anomaly as due to warping of the galactic disk, and determined the warping structure of M51's disk using the tilted-ring method, assuming that the intrinsic rotation curve is normal. It is shown that the disk is nearly flat in the inner disk at a constant inclination angle, but the disk suddenly bends at radius 7.5 kpc by about 27$°$. The inclination angle, then, decreases monotonically outward reaching a perfect face-on ring at 18 kpc, beyond which the disk is warped in the opposite sense to the inner disk, resulting in apparent counter rotation.

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Shouta Oikawa, Yoshiaki Sofue. 2014-06-30. Rotation Curve Anomaly and Galactic Warp in M51. https://doi.org/10.1093/pasj%2Fpsu059

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