HSC 2404

0.57 UTI

0.61

C_N

1.0

C_dens

0.75

C_C3

0.25

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 72

Radius (P>50% members) 2.3 [arcmin]

C_N 0.61 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High 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 2404 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old 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 Old

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 2404 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	–	168.131	-59.698	0.275	-4.046	0.21	-13.193
Hu & Soubiran	2025	168.158	-59.708	–	–	–	–
Hunt & Reffert	2024	168.135	-59.697	0.268	-4.055	0.2	-8.079
Cavallo et al.	2024	168.158	-59.708	0.271	–	–	–
Hunt & Reffert	2023	168.135	-59.697	0.268	-4.055	0.2	-8.079

💡 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
Hu & Soubiran	2025	–	–	–	–	-0.200*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	616*	–	–
Cavallo et al.	2024	2.86	2.00	–	2138	-0.310	–	–	–
Hunt & Reffert	2023	3.31	2.48	2.46	286	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3355	100.0	168.13	-59.7	0.27	-4.05	0.2	-12.93	0.21

💡 Note: The % column shows the percentage of members that HSC 2404 shares with each listed object.

Visualization

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