HSC 1744

0.08 UTI

0.0

C_N

0.09

C_dens

0.25

C_C3

0.03

C_lit

1.0

C_dup

N_m (P>50%) 18

Core radius and density 2.4 [pc], 0.5 [pc^-2]

C3 classification DB

C_N 0.0 Sparse
C_dens 0.09 Very loose
C_C3 0.25 Low quality
C_lit 0.03 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

HSC 1744 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate 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.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

🔍 Search references for HSC 1744 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	106.634	-7.865	0.387	-1.477	0.805	–
Hunt & Reffert	2024	106.621	-7.883	0.392	-1.487	0.786	–
Cavallo et al.	2024	106.635	-7.875	0.391	–	–	–
Hunt & Reffert	2023	106.621	-7.883	0.392	-1.487	0.786	–

💡 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]	B_frac	BSS
UCC	99999–	2.3	2.06	0.34	95	-0.010	128	–	–
Hunt & Reffert	2024	2.30	2.06	0.34	95	–	128⁽¹⁾	–	–
Cavallo et al.	2024	2.63	2.45	–	155	-0.010	–	–	–
Hunt & Reffert	2023	2.30	2.06	0.34	95	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

ℹ️

1 2