HSC 2365

0.00 UTI

0.29

C_N

0.76

C_dens

0.5

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BB

Number of members (P>50%) 29

Radius (P>50% members) 0.7 [arcmin]

C_N 0.29 Poorly populated
C_dens 0.76 Dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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HSC 2365 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a very large^* distance, well below the mid-plane, affected by low extinction. It is catalogued as a very old cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~13.57 kpc) differs significantly from the median photometric distance (~5.31 kpc).

Very distant Low extinction Very old

Data

🔍 Search references for HSC 2365 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	–	153.735	-64.611	0.074	-3.531	2.743	57.311
Hunt & Reffert	2024	153.735	-64.617	0.176	-3.505	2.741	–
Hunt & Reffert	2023	153.735	-64.617	0.176	-3.505	2.741	–

💡 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	–	–	–	–	–	738*	–	–
Hunt & Reffert	2023	5.31	0.61	1.04	7534	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
ESO 092 18	100.0	153.74	-64.61	0.05	-3.55	2.74	55.45	0.86

💡 Note: The % column shows the percentage of members that HSC 2365 shares with each listed object.

Visualization

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