Open cluster dissolution rate and the initial cluster mass function in the solar neighbourhood - Modelling the age and mass distributions of clusters observed by Gaia

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Volume 693 (January 2025)

A&A, 693 (2025) A305

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Table 4

Determined radii, masses, uncertainties, and quality flags for ten randomly selected OCs.

Name	r_c (pc)	$σ_{r_{c}}^{-}$ $\sigma _{{r_c}}^ -$ (pc)	$σ_{r_{c}}^{+}$ $\sigma _{{r_c}}^ +$ (pc)	r_k (pc)	$σ_{r_{k}}^{-}$ $\sigma _{{r_k}}^ -$ (pc)	$σ_{r_{k}}^{+}$ $\sigma _{{r_k}}^ +$ (pc)	M(r_k) (M_⊙)	σ_M (M_⊙)	M_f	P_f	R_f
UPK 640	3.58	0.32	0.47	12.38	2.51	3.27	419.32	8.24	1	1	1
Alessi 12	8.67	1.78	1.26	11.32	0.86	2.18	416.12	12.14	1	1	2
Roslund 3	1.01	0.09	0.12	37.49	25.66	40.20	399.38	13.25	1	1	2
NGC 3572	3.92	1.80	1.55	7.33	1.45	30.88	659.22	30.74	2	2	2
King 19	1.80	0.40	0.98	7.00	3.21	26.37	1100.31	31.83	1	2	1
NGC 6268	1.38	0.16	0.18	5.98	1.55	3.24	447.01	15.93	2	1	1
NGC 6259	2.24	0.11	0.12	31.08	9.71	21.27	5055.92	51.55	2	2	1
IC 1369	1.26	0.11	0.14	6.71	1.59	2.91	1374.01	35.58	1	2	1
Haffner 8	3.51	0.99	0.72	4.83	0.69	1.82	553.01	15.84	1	1	2
Berkeley 39	4.51	0.47	0.70	11.47	1.71	2.21	6456.33	167.55	1	1	1

Notes. Columns 2–7 include the structural parameters core radius (r_c) and King radius (r_k) with their respective lower and upper uncertainties (σ⁻, σ⁺, respectively). The mass within the King radius, M(r_k), and its uncertainty, σ_M, are in columns 8–9. The visually assigned classifications for the mass, photometry, and radii (M_f, P_f, R_f, respectively) are in columns 10–12. We also include the positions, ages, distances, and A_v from the Dias et al. (2021) catalogue and the values with respective uncertainties for parameters c and N₀ in the full table. An additional column with the assigned sample is also provided (2 = gold sample; ≥1 silver sample; ≥0 full sample). The full table with all 1724 OCs is available at the CDS.

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