HSC 1464

0.28 UTI

0.66

C_N

0.61

C_dens

0.75

C_C3

0.0

C_lit

0.7

C_dup

C3 classification AB

Number of members (P>50%) 82

Radius (P>50% members) 3.0 [arcmin]

C_N 0.66 Moderately populated
C_dens 0.61 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.7 Likely unique

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

Overview

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HSC 1464 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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 Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 1464 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	–	90.275	25.593	0.168	0.266	-0.43	–
Hunt & Reffert	2024	90.285	25.594	0.167	0.285	-0.461	25.558
Cavallo et al.	2024	90.258	25.588	0.17	–	–	–
Hunt & Reffert	2023	90.285	25.594	0.167	0.285	-0.461	25.558

💡 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	–	–	–	–	–	955*	–	–
Cavallo et al.	2024	4.06	1.65	–	132	0.250	–	–	–
Hunt & Reffert	2023	5.22	1.90	1.41	59	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0303	30.5	90.29	25.59	0.15	0.23	-0.41	–	0.35

💡 Note: The % column shows the percentage of members that HSC 1464 shares with each listed object.

Visualization

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