HSC 1652

0.47 UTI

0.49

C_N

1.0

C_dens

0.38

C_C3

0.25

C_lit

1.0

C_dup

C3 classification CB

Number of members (P>50%) 49

Radius (P>50% members) 1.5 [arcmin]

C_N 0.49 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

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HSC 1652 is a poorly populated, very dense object of low 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 1652 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	–	101.428	2.994	0.207	-0.445	0.807	–
Zhang et al.	2024	101.425	2.993	–	–	–	–
Hunt & Reffert	2024	101.425	2.993	0.224	-0.464	0.79	59.04
Cavallo et al.	2024	101.435	2.988	0.219	–	–	–
Hunt & Reffert	2023	101.425	2.993	0.224	-0.464	0.79	59.04

💡 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
Zhang et al.	2024	–	–	–	–	0.154*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	536*	–	–
Cavallo et al.	2024	5.30	2.29	–	257	0.010	–	–	–
Hunt & Reffert	2023	3.82	2.07	2.60	148	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3103	95.9	101.43	2.99	0.21	-0.43	0.8	57.66	0.09

💡 Note: The % column shows the percentage of members that HSC 1652 shares with each listed object.

Visualization

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