HXHWL 24

0.37 UTI

0.47

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 47

Stellar density (N₅₀/rad) 5.8 [N/pc²]

C3 classification CB

C_N 0.47 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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HXHWL 24 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Data

🔍 Search references for HXHWL 24 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–	116.315	-20.066	0.604	-1.009	0.618	-6.159
He et al.	2021	116.3	-20.061	0.59	-0.99	0.59	–

💡 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–	1.74	1.2	–	91	0.498	–	–	–
He et al.	2021	1.74	1.20	–	91	0.498	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 3229	95.7	116.31	-20.05	0.61	-1.0	0.62	-6.16	0.03

💡 Note: The % column shows the percentage of members that HXHWL 24 shares with each listed object.

Visualization

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