HSC 2392

0.32 UTI

0.0

C_N

0.59

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 22

Stellar density (N₅₀/rad) 2.9 [N/pc²]

C3 classification AA

C_N 0.0 Sparse
C_dens 0.59 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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HSC 2392 is a sparse, moderately dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Very distant Moderate extinction Metal-poor Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 2392 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–	163.257	-61.288	0.17	-4.882	1.786	2.072
Hunt & Reffert	2024	163.233	-61.291	0.172	-4.896	1.788	–
Cavallo et al.	2024	163.25	-61.289	0.171	–	–	–
Hunt & Reffert	2023	163.233	-61.291	0.172	-4.896	1.788	–

💡 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–	5.23	1.575	0.98	186	-0.570	217	–	–
Hunt & Reffert	2024	–	–	–	–	–	217⁽¹⁾	–	–
Cavallo et al.	2024	5.13	1.64	–	182	-0.570	–	–	–
Hunt & Reffert	2023	5.33	1.51	0.98	189	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3364	96.0	163.26	-61.29	0.17	-4.88	1.79	2.07	0.01

💡 Note: The % column shows the percentage of members that HSC 2392 shares with each listed object.

Visualization

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