HSC 2514

0.26 UTI

0.0

C_N

0.41

C_dens

0.75

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 24

Core radius and density 1.0 [pc], 2.0 [pc^-2]

C3 classification AB

C_N 0.0 Sparse
C_dens 0.41 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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HSC 2514 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Relatively close Low extinction Near-solar metallicity Young

Liu et al. (2025)
Classified as primordial binary cluster 116 along with CWNU_2405.

Palma et al. (2025)
Classified as genetic pair P202, along with CWNU_2405.

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 HSC 2514 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–	186.233	-65.203	0.418	-5.167	-0.46	9.851
Hunt & Reffert	2024	186.281	-65.209	0.416	-5.173	-0.462	9.821
Cavallo et al.	2024	186.1	-65.163	0.416	–	–	–
Hunt & Reffert	2023	186.281	-65.209	0.416	-5.173	-0.462	9.821

💡 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–	2.28	0.79	1.66	37	0.090	196	–	–
Liu et al.	2025	3.27	0.33	–	20	–	–	–	–
Hunt & Reffert	2024	2.22	0.79	1.66	37	–	196⁽¹⁾	–	–
Cavallo et al.	2024	2.34	1.03	–	45	0.090	–	–	–
Hunt & Reffert	2023	2.22	0.79	1.66	37	–	–	–	–

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

Visualization

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