HSC 1356

0.08 UTI

0.37

C_N

1.0

C_dens

0.38

C_C3

0.25

C_lit

0.19

C_dup

C3 classification CB

Number of members (P>50%) 37

Radius (P>50% members) 3.4 [arcmin]

C_N 0.37 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.25 Poorly studied
C_dup 0.19 Likely duplicate

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

Overview

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HSC 1356 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 metal-rich, very young cluster (see Parameters). It was recently reported in the literature.

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

Relatively close Moderate extinction Metal-rich Very young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 1356 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	–	81.863	34.387	0.461	0.169	-1.868	79.387
Zhang et al.	2024	81.867	34.373	–	–	–	–
Hunt & Reffert	2024	81.867	34.373	0.459	0.162	-1.866	79.412
Cavallo et al.	2024	81.909	34.387	0.458	–	–	–
Hunt & Reffert	2023	81.867	34.373	0.459	0.162	-1.866	79.412

💡 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	–	–	–	–	–	397*	–	–
Cavallo et al.	2024	2.37	1.56	–	21	0.500	–	–	–
Hunt & Reffert	2023	2.07	1.55	2.10	14	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Stock 8	81.1	81.96	34.43	0.46	0.08	-2.34	-59.37	0.91

💡 Note: The % column shows the percentage of members that HSC 1356 shares with each listed object.

Visualization

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