Abstract
As globular clusters (GCs) orbit the Milky Way, their stars are tidally stripped forming tidal tails that follow the orbit of the cluster around the
Galaxy. The morphology of these tails is complex and shows correlations with the phase of orbit and the orbital angular velocity, especially for
GCs on eccentric orbits. Here, we focus on two GCs, NGC 1261 and NGC 1904, that have potentially been accreted alongside Gaia-Enceladus and
that have shown signatures of having, in addition to tidal tails, structures formed by distributions of extra-tidal stars that are misaligned with the
general direction of the clusters’ respective orbits. To provide an explanation for the formation of these structures, we make use of spectroscopic
measurements from the Southern Stellar Stream Spectroscopic Survey (S
5
) as well as proper motion measurements from Gaia’s third data release
(DR3), and apply a Bayesian mixture modelling approach to isolate high-probability member stars. We recover extra-tidal features similar to
those found in Shipp et al. (2018) surrounding each cluster. We conduct N-body simulations and compare the expected spatial distribution and
variation in the dynamical parameters along the orbit with those of our potential member sample. Furthermore, we use Dark Energy Camera
(DECam) photometry to inspect the distribution of the member stars in the colour-magnitude diagram (CMD). We find that potential members
agree reasonably with the N-body simulations and that the majority of them follow a simple stellar population-like distribution in the CMD which
is characteristic of GCs. We link the extra-tidal features with their orbital properties and find that the presence of the tails agrees well with the
theory of stellar stream formation through tidal disruption. In the case of NGC 1904, we clearly detect the tidal debris escaping the inner and outer
Lagrange points which are expected to be prominent when at or close to the apocenter of its orbit. Our analysis allows for further exploration of
other GCs in the Milky Way that exhibit similar extra-tidal features.