HSC 1704

0.43 UTI

0.4

C_N

0.86

C_dens

0.38

C_C3

0.25

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 40

Radius (P>50% members) 1.9 [arcmin]

C_N 0.4 Poorly populated
C_dens 0.86 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 1704 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a large distance, below 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.

Very distant Moderate extinction Near-solar metallicity Old

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 1704 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	–	103.101	-3.311	0.181	-0.084	0.043	53.239
Hu & Soubiran	2025	103.104	-3.322	–	–	–	–
Hunt & Reffert	2024	103.084	-3.314	0.173	-0.122	0.06	63.259
Cavallo et al.	2024	103.104	-3.322	0.171	–	–	–
Hunt & Reffert	2023	103.084	-3.314	0.173	-0.122	0.06	63.259

💡 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	–	–	–	–	-0.290*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	532*	–	–
Cavallo et al.	2024	5.55	2.02	–	1380	-0.460	–	–	–
Hunt & Reffert	2023	4.68	1.91	1.17	776	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3345	80.0	103.1	-3.31	0.18	-0.09	0.01	53.13	0.07

💡 Note: The % column shows the percentage of members that HSC 1704 shares with each listed object.

Visualization

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