UBC 1595

0.30 UTI

0.37

C_N

0.27

C_dens

0.75

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 37

Core radius and density 1.4 [pc], 1.4 [pc^-2]

C3 classification AB

C_N 0.37 Poorly populated
C_dens 0.27 Loose
C_C3 0.75 High quality
C_lit 0.06 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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UBC 1595 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

Close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

🔍 Search references for UBC 1595 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	289.961	-1.895	1.063	-0.779	-2.135	4.963
Hunt & Reffert	2024	289.951	-1.872	1.069	-0.797	-2.153	-20.105
Cavallo et al.	2024	289.936	-1.934	1.069	–	–	–
Hunt & Reffert	2023	289.951	-1.872	1.069	-0.797	-2.153	-20.105
Castro-Ginard et al.	2022	289.95	-1.87	1.07	-0.78	-2.12	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	B_frac	BSS
UCC	99999–	0.96	1.93	0.9	33	0.080	130	–	–
Hunt & Reffert	2024	0.89	1.73	0.90	33	–	130⁽¹⁾	–	–
Cavallo et al.	2024	1.04	2.33	–	32	0.080	–	–	–
Hunt & Reffert	2023	0.89	1.73	0.90	33	–	–	–	–
Castro-Ginard et al.	2022	1.03	2.13	–	126	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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