HSC 914

0.46 UTI

0.31

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 31

Stellar density (N₅₀/rad) 12.6 [N/pc²]

C3 classification AA

C_N 0.31 Poorly populated
C_dens 1.0 Very 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 914 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, 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.

Distant High extinction Massive Metal-rich Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 914 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–	353.727	63.365	0.223	-1.941	-0.527	-84.936
Hunt & Reffert	2024	353.726	63.372	0.225	-1.941	-0.541	-84.938
Cavallo et al.	2024	353.75	63.364	0.225	–	–	–
Hunt & Reffert	2023	353.726	63.372	0.225	-1.941	-0.541	-84.938

💡 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–	3.705	3.925	2.34	328	0.590	1019	–	–
Hunt & Reffert	2024	–	–	–	–	–	1019⁽¹⁾	–	–
Cavallo et al.	2024	3.60	3.56	–	398	0.590	–	–	–
Hunt & Reffert	2023	3.81	4.29	2.34	258	–	–	–	–

(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 3362	100.0	353.73	63.37	0.22	-1.94	-0.52	-84.94	0.15

💡 Note: The % column shows the percentage of members that HSC 914 shares with each listed object.

Visualization

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