HXHWL 32

(H21OC 32)

0.47 UTI

0.58

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 66

Stellar density (N₅₀/rad) 5.3 [N/pc²]

C3 classification AB

C_N 0.58 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High 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 32 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for HXHWL 32 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–	105.681	-7.744	0.876	-1.588	-3.484	6.472
He et al.	2022	105.691	-7.724	0.882	-1.565	-3.487	–
He et al.	2021	105.664	-7.746	0.88	-1.59	-3.46	–

💡 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–	1.26	0.93	–	252	0.498	–	–	–
He et al.	2022	–	0.90	–	158	–	–	–	–
He et al.	2021	1.26	0.96	–	347	0.498	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CMa02	98.5	105.68	-7.75	0.88	-1.59	-3.48	5.88	0.01
CWWDL 14378	77.3	105.68	-7.72	0.88	-1.58	-3.48	5.88	0.0

💡 Note: The % column shows the percentage of members that HXHWL 32 shares with each listed object.

Visualization

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