HSC 406

0.04 UTI

0.0

C_N

0.09

C_dens

0.25

C_C3

0.0

C_lit

0.56

C_dup

C3 classification DB

Number of members (P>50%) 19

Radius (P>50% members) 6.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.09 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.56 Likely unique

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

Overview

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HSC 406 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Bronze sample.

Data

🔍 Search references for HSC 406 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	–	290.252	13.604	0.317	-1.572	-4.535	24.117
Hunt & Reffert	2024	290.289	13.588	0.318	-1.587	-4.503	24.095
Cavallo et al.	2024	290.263	13.591	0.321	–	–	–
Hunt & Reffert	2023	290.289	13.588	0.318	-1.587	-4.503	24.095

💡 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	–	–	–	–	–	967*	–	–
Cavallo et al.	2024	3.75	4.67	–	12	-0.090	–	–	–
Hunt & Reffert	2023	2.79	4.95	2.69	14	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 0126	44.0	290.27	13.7	0.32	-1.61	-4.53	18.9	0.3

💡 Note: The % column shows the percentage of members that HSC 406 shares with each listed object.

Visualization

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