HSC 708

0.31 UTI

0.28

C_N

1.0

C_dens

0.25

C_C3

0.0

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 28

Radius (P>50% members) 6.3 [arcmin]

C_N 0.28 Poorly populated
C_dens 1.0 Very dense
C_C3 0.25 Low 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 708 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near 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 object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 708 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	–	320.766	46.249	0.797	0.7	-2.694	–
Hunt & Reffert	2024	320.753	46.26	0.803	0.685	-2.724	–
Cavallo et al.	2024	320.744	46.258	0.803	–	–	–
Hunt & Reffert	2023	320.753	46.26	0.803	0.685	-2.724	–

💡 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	–	–	–	–	–	99*	–	–
Cavallo et al.	2024	1.39	1.70	–	19	0.060	–	–	–
Hunt & Reffert	2023	1.21	1.75	1.35	48	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3021	89.3	320.77	46.26	0.8	0.71	-2.69	–	0.03

💡 Note: The % column shows the percentage of members that HSC 708 shares with each listed object.

Visualization

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