HSC 1286

0.42 UTI

0.34

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 34

Radius (P>50% members) 1.1 [arcmin]

C_N 0.34 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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HSC 1286 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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 Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 1286 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	–	77.075	42.748	0.185	0.291	-0.389	-18.719
Hunt & Reffert	2024	77.069	42.747	0.187	0.294	-0.411	–
Cavallo et al.	2024	77.067	42.748	0.19	–	–	–
Hunt & Reffert	2023	77.069	42.747	0.187	0.294	-0.411	–

💡 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]	Bfr	BSS
Hunt & Reffert	2024	–	–	–	–	–	365*	–	–
Cavallo et al.	2024	4.79	1.69	–	46	-0.010	–	–	–
Hunt & Reffert	2023	4.53	1.39	0.90	204	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3018	100.0	77.08	42.75	0.21	0.3	-0.39	-18.72	0.29

💡 Note: The % column shows the percentage of members that HSC 1286 shares with each listed object.

Visualization

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