HSC 1472

0.38 UTI

0.25

C_N

0.92

C_dens

0.62

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 25

Core radius and density 0.7 [pc], 4.6 [pc^-2]

C3 classification AC

C_N 0.25 Poorly populated
C_dens 0.92 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.06 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 1472 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Wood sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.08 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.08 (50th percentile).

Data

🔍 Search references for HSC 1472 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–	86.151	21.861	0.737	0.986	-2.962	14.763
Zhang et al.	2024	86.146	21.847	–	–	–	–
Hunt & Reffert	2024	86.146	21.847	0.733	0.988	-2.959	18.094
Cavallo et al.	2024	86.149	21.863	0.731	–	–	–
Hunt & Reffert	2023	86.146	21.847	0.733	0.988	-2.959	18.094

💡 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–	1.31	1.82	1.44	87	0.023	89	–	–
Zhang et al.	2024	–	–	–	–	0.066⁽¹⁾	–	–	–
Hunt & Reffert	2024	1.31	1.82	1.44	87	–	89⁽¹⁾	–	–
Cavallo et al.	2024	1.45	0.87	–	1023	-0.020	–	–	–
Hunt & Reffert	2023	1.31	1.82	1.44	87	–	–	–	–

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

Visualization

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