HSC 1776

0.13 UTI

0.0

C_N

0.16

C_dens

0.5

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 20

Radius (P>50% members) 4.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.16 Very loose
C_C3 0.5 Intermediate 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 1776 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low 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.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 1776 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	–	110.535	-10.694	0.259	-1.454	0.745	–
Hunt & Reffert	2024	110.5	-10.688	0.264	-1.441	0.759	–
Cavallo et al.	2024	110.515	-10.698	0.264	–	–	–
Hunt & Reffert	2023	110.5	-10.688	0.264	-1.441	0.759	–

💡 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	–	–	–	–	–	179*	–	–
Cavallo et al.	2024	2.88	0.71	–	398	0.020	–	–	–
Hunt & Reffert	2023	3.40	0.67	0.62	316	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3014	88.0	110.52	-10.69	0.26	-1.45	0.75	–	0.02

💡 Note: The % column shows the percentage of members that HSC 1776 shares with each listed object.

Visualization

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