HSC 2450

0.07 UTI

0.0

C_N

0.4

C_dens

0.38

C_C3

0.0

C_lit

0.48

C_dup

N₅₀ (P>50% members) 18

Stellar density (N₅₀/rad) 2.0 [N/pc²]

C3 classification CB

C_N 0.0 Sparse
C_dens 0.4 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.48 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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HSC 2450 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for HSC 2450 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–	175.957	-60.512	0.273	-7.911	1.782	–
Hunt & Reffert	2024	175.972	-60.513	0.321	-7.925	1.781	–
Hunt & Reffert	2023	175.972	-60.513	0.321	-7.925	1.781	–

💡 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–	2.92	1.31	0.95	887	–	211	–	–
Hunt & Reffert	2024	–	–	–	–	–	211⁽¹⁾	–	–
Hunt & Reffert	2023	2.92	1.31	0.95	887	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CKCWDM 48869	60.0	175.98	-60.53	0.18	-7.87	1.76	-4.19	0.05
UBC 1505	52.0	175.99	-60.53	0.17	-7.88	1.77	2.8	0.62

💡 Note: The % column shows the percentage of members that HSC 2450 shares with each listed object.

Visualization

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