HSC 2386

0.46 UTI

0.57

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BA

Number of members (P>50%) 64

Radius (P>50% members) 1.9 [arcmin]

C_N 0.57 Moderately 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 2386 is a moderately populated, very dense 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, 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)
Silver sample.

Data

🔍 Search references for HSC 2386 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	–	164.262	-59.694	0.2	-4.565	2.139	15.356
Hunt & Reffert	2024	164.259	-59.692	0.2	-4.582	2.135	17.494
Cavallo et al.	2024	164.265	-59.686	0.2	–	–	–
Hunt & Reffert	2023	164.259	-59.692	0.2	-4.582	2.135	17.494

💡 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	–	–	–	–	–	959*	–	–
Cavallo et al.	2024	3.55	2.64	–	490	-0.290	–	–	–
Hunt & Reffert	2023	4.39	2.48	2.48	254	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3337	95.3	164.26	-59.69	0.2	-4.57	2.14	15.2	0.03

💡 Note: The % column shows the percentage of members that HSC 2386 shares with each listed object.

Visualization

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