HXHWL 73

0.39 UTI

0.36

C_N

0.82

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 36

Radius (P>50% members) 7.2 [arcmin]

C_N 0.36 Poorly populated
C_dens 0.82 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 73 is a poorly populated, dense object of high 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 2 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Data

🔍 Search references for HXHWL 73 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	–	62.689	57.137	0.706	0.983	-1.084	-29.84
He et al.	2021	62.692	57.153	0.69	1.04	-1.06	–

💡 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.	2021	1.20	2.52	–	66	0.169	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 12760	100.0	62.69	57.14	0.71	0.95	-1.08	-29.84	0.17
Theia 7938	100.0	62.68	57.14	0.71	0.95	-1.08	-29.84	0.02

💡 Note: The % column shows the percentage of members that HXHWL 73 shares with each listed object.

Visualization

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