HSC 1093

0.40 UTI

0.0

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 23

Radius (P>50% members) 0.8 [arcmin]

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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HSC 1093 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~7.43 kpc) differs significantly from the median photometric distance (~4.54 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant Moderate extinction Metal-poor Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 1093 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	–	39.832	64.618	0.135	-1.379	0.495	–
Hunt & Reffert	2024	39.826	64.619	0.13	-1.385	0.496	–
Cavallo et al.	2024	39.844	64.619	0.135	–	–	–
Hunt & Reffert	2023	39.826	64.619	0.13	-1.385	0.496	–

💡 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	–	–	–	–	–	365*	–	–
Cavallo et al.	2024	2.99	2.90	–	151	-0.860	–	–	–
Hunt & Reffert	2023	6.08	2.59	0.60	24	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3168	100.0	39.85	64.62	0.12	-1.39	0.5	–	0.12

💡 Note: The % column shows the percentage of members that HSC 1093 shares with each listed object.

Visualization

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