The spiral structure of the Galaxy revealed by CS sources and evidence for the 4:1 resonance
J.R.D. Lepine, A. Roman-Lopes, Zulema Abraham, T.C. Junqueira, Yu. N., Mishurov

TL;DR
This study maps the Galaxy's spiral structure using CS emission from IRAS sources, revealing well-defined arms, a 4:1 resonance sub-structure, and new features consistent with galactic dynamics and star formation regions.
Contribution
It provides a detailed spiral map based on molecular CS sources, identifying a resonance-related sub-structure and new spiral features, expanding understanding of galactic morphology.
Findings
Spiral arms confined inside co-rotation radius.
Identification of a square-shaped sub-structure at the 4:1 resonance.
Discovery of a new concave curvature arm in Sagitta to Cepheus region.
Abstract
We present a map of the spiral structure of the Galaxy, as traced by molecular CS emission associated with IRAS sources which are believed to be compact HII regions. The CS line velocities are used to determine the kinematic distances of the sources, in order to investigate their distribution in the galactic plane. This allows us to use 870 objects to trace the arms, a number larger than that of previous studies based on classical HII regions. The distance ambiguity of the kinematic distances, when it exists, is solved by different procedures, including the latitude distribution and an analysis of the longitude-velocity diagram. The well defined spiral arms are seen to be confined inside the co-rotation radius, as is often the case in spiral galaxies. We identify a square-shaped sub-structure in the CS map with that predicted by stellar orbits at the 4:1 resonance (4 epicycle…
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