HSC 2424

0.24 UTI

0.34

C_N

0.37

C_dens

0.5

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 34

Stellar density (N₅₀/rad) 1.8 [N/pc²]

C3 classification BB

C_N 0.34 Poorly populated
C_dens 0.37 Loose
C_C3 0.5 Intermediate 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 2424 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-poor, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~4.35 kpc) differs significantly from the median photometric distance (~2.93 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High extinction Metal-poor Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 2424 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–	169.719	-61.652	0.23	-6.084	1.561	–
Hunt & Reffert	2024	169.704	-61.622	0.228	-6.075	1.579	–
Cavallo et al.	2024	169.726	-61.65	0.226	–	–	–
Hunt & Reffert	2023	169.704	-61.622	0.228	-6.075	1.579	–

💡 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–	2.93	3.015	2.7	114	-0.680	753	–	–
Hunt & Reffert	2024	–	–	–	–	–	753⁽¹⁾	–	–
Cavallo et al.	2024	2.25	2.95	–	209	-0.680	–	–	–
Hunt & Reffert	2023	3.61	3.08	2.70	18	–	–	–	–

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

Visualization

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