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EWOCS-XI: Anisotropic expansion and shear in the cluster Westerlund 1. A 2D kinematic analysis with Gaia DR3

Westerlund 1 (Wd1) is one of the Milky Way's most massive young clusters, in which heavy extinction and field contamination have historically hampered its kinematic characterization.

By Prisinzano, Damiani, Ordenes-Huanca +14

Score████░░░░░░4.3

VerdictWorth a reader's time today.

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Abstract

Westerlund 1 (Wd1) is one of the Milky Way's most massive young clusters, in which heavy extinction and field contamination have historically hampered its kinematic characterization. We aim to assess Wd1's internal kinematics, dynamical state, and formation scenario. Using a robust 5D clustering approach, we identified 559 bona fide members. We modeled their proper motions via a 2D first-order Taylor expansion to derive the velocity gradient tensor, mapping expansion, rotation, and shear. Restricting the kinematic analysis to 524 stars with proper motion uncertainties 4σ$) highlighting preferred expansion along the Galactic latitude (position angle $164^\circ\pm10.1^\circ$). A detected cross-gradient ($\partial v_b / \partial l = -0.41 ± 0.08 km s^{-1} pc^{-1}$) provides a clear signature of shear on the plane of the sky. Wd1 does not behave as a single cohesive population, but comprises two decoupled subsystems: a stable, bound core in dynamical equilibrium and an escaping, unbound envelope. This prominent anisotropic expansion perpendicular to the Galactic plane has a kinematic timescale (Δt_kin = 2.08 ± 0.44 Myr) matching the independent orbital mid-plane crossing time (Δt_orbit = 2.10 ± 0.05 Myr). This temporal alignment indicates the expansion onset coincided with Wd1's Galactic disk passage, triggered either by internal dynamics (e.g., early supernova feedback) or external tidal perturbations. Finally, the robust unbound population demonstrates that active cluster dissolution is underway, driven by discrete dynamical ejection events rather than long-term stellar evaporation.

L. Prisinzano, F. Damiani, C. Ordenes-Huanca, M. Tarantino, S. Sciortino, N. J. Wright, V. Almendros-Abad, M. Andersen, A. Bayo, R. Bonito, V. Cusimano, M. Haberle, K. Mužic, I. Negueruela, E. Sabbi, A. Winter, M. G. Guarcello

The editor's rubric

Heuristic review

DimensionLevelWeightWhat that level means
Leverage███░░ 318%A method or resource many groups across the field will adopt within a year.
Magnitude██░░░ 220%Solid incremental gain on a meaningful problem.
Evidence███░░ 322%Solid: multiple benchmarks or cohorts, ablations, fair baselines, released code or data.
Novelty███░░ 322%A genuinely new approach to an open problem.
Trajectory██░░░ 210%Some room to improve with obvious engineering.
Stakes██░░░ 28%Benefits a professional community (practitioners, clinicians, engineers).

Editor’s rationale

Heuristic triage from title and abstract text only, not a reading of the paper. Cues found: method (we report); novelty (alternative to status quo); verification (error bars, independent replication).

How the score was computed

rank-2026-10-07

Score████░░░░░░4.3

Score = 10 × (75% × adjusted merit / 10 + 15% × attention + 10% × freshness)

Merit
5.2 / 10
Weighted rubric, evidence-gated.
Adjusted merit
4.5 / 10
Shrunk toward the desk prior by editor confidence (38%).
Attention
0%
Citations, upvotes, points, mentions.
Freshness
94%
Half-life decay since publication.

No attention signals recorded yet.

The record

  • Reviewed by heuristic-v5 on Oct 9, 2026, 07:29 UTC. Paper type: method.
  • Categories: astro-ph.SR, astro-ph.GA
  • BRIEF, No.8 in the Physics edition of October 9, 2026.