HSC 2527

0.19 UTI

0.0

C_N

0.15

C_dens

0.75

C_C3

0.03

C_lit

1.0

C_dup

N_m (P>50%) 17

Core radius and density 2.0 [pc], 0.7 [pc^-2]

C3 classification AB

C_N 0.0 Sparse
C_dens 0.15 Very loose
C_C3 0.75 High 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

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HSC 2527 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by very high extinction. It is catalogued as a near-solar metallicity, very 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.

Distant Very high extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Bronze sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.04 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.04 (50th percentile).

Data

🔍 Search references for HSC 2527 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	99999–	190.395	-62.028	0.251	-6.347	-0.161	–
Hunt & Reffert	2024	190.403	-62.044	0.243	-6.436	-0.113	–
Cavallo et al.	2024	190.512	-61.93	0.245	–	–	–
Hunt & Reffert	2023	190.403	-62.044	0.243	-6.436	-0.113	–

💡 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–	3.86	5.02	2.9	19	0.350	320	–	–
Hunt & Reffert	2024	3.86	5.02	2.90	19	–	320⁽¹⁾	–	–
Cavallo et al.	2024	3.68	4.64	–	13	0.350	–	–	–
Hunt & Reffert	2023	3.86	5.02	2.90	19	–	–	–	–

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

Visualization

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