HXHWL 26

(H21OC 26)

0.43 UTI

0.76

C_N

0.62

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 121

Radius (P>50% members) 17.5 [arcmin]

C_N 0.76 Rich
C_dens 0.62 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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HXHWL 26 is a rich, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It is rarely studied in the literature.

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

Relatively close Low extinction Metal-rich Young

Data

🔍 Search references for HXHWL 26 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	–	111.565	-26.602	0.816	-4.267	3.901	37.343
He et al.	2022	111.493	-26.51	0.812	-4.246	3.913	–
He et al.	2021	111.646	-26.584	0.8	-4.29	3.85	–

💡 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]	Bfr	BSS
He et al.	2022	–	0.20	–	32	–	–	–	–
He et al.	2021	1.26	0.12	–	28	0.537	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2267	33.1	111.14	-26.52	0.82	-4.23	3.95	37.01	0.15
CWWDL 14101	26.4	111.61	-26.56	0.82	-4.26	3.9	38.66	0.0

💡 Note: The % column shows the percentage of members that HXHWL 26 shares with each listed object.

Visualization

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