Evolution of the local spiral structure of the Milky Way revealed by
  open clusters
  The structure and evolution of the spiral arms of our Milky Way are basic but
long-standing questions in astronomy. In particular, the lifetime of spiral
arms is still a puzzle and has not been well constrained from observations. In
this work, we aim to inspect these issues using a large catalogue of open
clusters. We compiled a catalogue of 3794 open clusters based on Gaia EDR3. A
majority of these clusters have accurately determined parallaxes, proper
motions, and radial velocities. The age parameters for these open clusters are
collected from references or calculated in this work. In order to understand
the nearby spiral structure and its evolution, we analysed the distributions,
kinematic properties, vertical distributions, and regressed properties of
subsamples of open clusters. We find evidence that the nearby spiral arms are
compatible with a long-lived spiral pattern and might have remained
approximately stable for the past 80 million years. In particular, the Local
Arm, where our Sun is currently located, is also suggested to be long-lived in
nature and probably a major arm segment of the Milky Way. The evolutionary
characteristics of nearby spiral arms show that the dynamic spiral mechanism
might be not prevalent for our Galaxy. Instead, density wave theory is more
consistent with the observational properties of open clusters.
