Disentangling the Arcturus stream
Iryna Kushniruk, Thomas Bensby

TL;DR
This study analyzes the kinematic and chemical properties of the Arcturus stream and other stellar groups using Gaia DR2 data, suggesting they are remnants of an ancient merger rather than a dissolved cluster or bar-related structures.
Contribution
It provides a detailed kinematic and chemical analysis of multiple stellar streams, proposing that the Arcturus stream is likely a phase-space wave from an ancient merger event.
Findings
Arcturus, AF06, and KFR08 streams are low-velocity, thick disk-like structures.
Streams are detected in steps of 20-30 km/s in azimuthal velocity.
Chemical diversity indicates they are not dissolved open clusters.
Abstract
The Arcturus stream is an over-density of stars in velocity space and its origin has been much debated recently without any clear conclusion. Resolving the nature of the Arcturus stream can provide clues to the formation history of the Milky Way and its stellar populations. The space velocities, angular momenta and actions for a sample of more than 5.8 million stars, composed from Gaia DR2, are analysed with a wavelet transform. The kinematic characteristics of each identified group is used to select possible members of the groups from the GALAH and APOGEE spectroscopic surveys to further study and constrain their chemical properties. In the velocity and angular momentum spaces the already known Sirius, Pleiades, Hyades, Hercules, AF06, Arcturus and KFR08 streams are clearly identified. The Hercules stream appears to be a mixture of thin and thick disk stars. The Arcturus stream, as…
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