HSC 1876

0.12 UTI

0.25

C_N

0.33

C_dens

0.75

C_C3

0.0

C_lit

0.44

C_dup

C3 classification AB

Number of members (P>50%) 25

Radius (P>50% members) 3.4 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.33 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

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

Overview

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HSC 1876 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Distant Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 1876 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	–	116.441	-19.186	0.256	-1.675	2.212	–
Hunt & Reffert	2024	116.435	-19.188	0.245	-1.648	2.201	–
Cavallo et al.	2024	116.403	-19.166	0.246	–	–	–
Hunt & Reffert	2023	116.435	-19.188	0.245	-1.648	2.201	–

💡 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	–	–	–	–	–	174*	–	–
Cavallo et al.	2024	3.56	0.56	–	417	0.100	–	–	–
Hunt & Reffert	2023	4.03	0.61	1.44	232	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 1414	56.0	116.44	-19.17	0.24	-1.72	2.24	–	0.13

💡 Note: The % column shows the percentage of members that HSC 1876 shares with each listed object.

Visualization

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