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Abstract We apply the automatic stellar stream detection algorithm StarStream to Gaia Data Release 3 and identify 87 stellar streams associated with Galactic globular clusters (GCs), including 34 high-quality cases with median completeness and purity both exceeding 50%, as estimated from modeling mock streams. These detections double the number of known GC streams and increase the fraction of GCs with tidal streams at high Galactic latitudes (∣ b ∣ > 30°) to 75%. In contrast to visual expectations, many new streams are wide or short, or misaligned with their progenitors’ orbits. Taking advantage of the unbiased density measurements enabled by our method, we also estimate the mass-loss rate for the progenitor GCs. We find that several low-mass, large-size clusters have enhanced mass-loss rates, indicating that they are approaching complete tidal disruption.
Chen et al. (Mon,) studied this question.