Burton’s Curse: The Impact of Bulk Flows on the Galactic Longitude–Velocity Diagram and the Illusion of a Continuous Perseus Arm - Archive ouverte HAL Accéder directement au contenu
Article Dans Une Revue The Astrophysical Journal Année : 2022

Burton’s Curse: The Impact of Bulk Flows on the Galactic Longitude–Velocity Diagram and the Illusion of a Continuous Perseus Arm

J. Peek
Kirill Tchernyshyov
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Abstract In this work, we demonstrate that the Perseus Arm is not a continuous structure of molecular gas in the second quadrant. We first show that the observed, distanced-resolved velocity structure of the Galaxy in the outer disk is capable of creating illusory spiral arms, as was first proposed by Burton. Second, we measure the distances to a collection of CO clouds at velocities consistent with the Perseus arm with 135° < l < 160°. We find these distances using 3D dust maps from Green et al. We determine that these molecular clouds do not preferentially lie at the distance of a purported Perseus arm but rather extend over 3 kpc in distance, with some evidence for a closer, high pitch angle structure between 1 and 1.5 kpc away. Finally, we demonstrate that velocity perturbations of the amplitude found near the Perseus arm can wreak havoc on our interpretation of the longitude–velocity diagram for more than half of the Milky Way disk.
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hal-03873389 , version 1 (27-11-2022)

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J. Peek, Kirill Tchernyshyov, Marc-Antoine Miville-Deschênes. Burton’s Curse: The Impact of Bulk Flows on the Galactic Longitude–Velocity Diagram and the Illusion of a Continuous Perseus Arm. The Astrophysical Journal, 2022, 925 (2), pp.201. ⟨10.3847/1538-4357/ac3f34⟩. ⟨hal-03873389⟩
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