HSC 1851

0.27 UTI

0.27

C_N

0.59

C_dens

0.5

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 27

Radius (P>50% members) 2.9 [arcmin]

C_N 0.27 Poorly populated
C_dens 0.59 Moderately dense
C_C3 0.5 Intermediate 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 1851 is a poorly populated, moderately dense object of intermediate 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, 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.

Distant Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 1851 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	–	113.986	-18.079	0.278	-1.715	2.013	92.756
Hunt & Reffert	2024	113.98	-18.091	0.263	-1.703	2.004	–
Cavallo et al.	2024	113.979	-18.082	0.261	–	–	–
Hunt & Reffert	2023	113.98	-18.091	0.263	-1.703	2.004	–

💡 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	–	–	–	–	–	338*	–	–
Cavallo et al.	2024	3.50	2.37	–	23	-0.090	–	–	–
Hunt & Reffert	2023	3.37	2.06	0.95	143	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3740	92.6	113.98	-18.08	0.28	-1.69	2.01	87.59	0.03

💡 Note: The % column shows the percentage of members that HSC 1851 shares with each listed object.

Visualization

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