HSC 1014

0.32 UTI

0.44

C_N

0.41

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 44

Stellar density (N₅₀/rad) 2.1 [N/pc²]

C3 classification AB

C_N 0.44 Poorly populated
C_dens 0.41 Loose
C_C3 0.75 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 1014 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young 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 Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 1014 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–	20.2	62.524	0.284	-1.583	-0.165	-29.747
Hunt & Reffert	2024	20.188	62.51	0.294	-1.578	-0.179	–
Cavallo et al.	2024	20.167	62.524	0.294	–	–	–
Hunt & Reffert	2023	20.188	62.51	0.294	-1.578	-0.179	–

💡 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–	3.28	2.52	1.9	12	0.160	599	–	–
Hunt & Reffert	2024	–	–	–	–	–	599⁽¹⁾	–	–
Cavallo et al.	2024	3.45	2.34	–	9	0.160	–	–	–
Hunt & Reffert	2023	3.11	2.70	1.90	14	–	–	–	–

(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 3577	100.0	20.18	62.52	0.28	-1.58	-0.17	-87.63	0.06

💡 Note: The % column shows the percentage of members that HSC 1014 shares with each listed object.

Visualization

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