Dynamical model of Praesepe and its tidal tails | Astronomy & Astrophysics (A&A)

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Table 4

Comparing distances of clumps via direct measurement and theoretical calculation.

Step (pc)	δL (kpc km s⁻¹)	d_step (pc)	y_T (pc)
−211	10.58	239	247
−450	10.88	250	254
−700	11.06	−	259

Notes. The distance to the next step from the one at −700 pc was not estimated, as at the end of the simulation the star had yet not passed through the entire step.

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