HXHWL 58

0.29 UTI

0.0

C_N

0.2

C_dens

0.75

C_C3

0.25

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 23

Radius (P>50% members) 7.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.2 Very loose
C_C3 0.75 High quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

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HXHWL 58 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HXHWL 58 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	–	98.937	8.762	0.483	-0.034	-1.365	–
Hunt & Reffert	2024	98.949	8.766	0.486	-0.04	-1.348	-14.737
Cavallo et al.	2024	98.907	8.753	0.489	–	–	–
Hunt & Reffert	2023	98.949	8.766	0.486	-0.04	-1.348	-14.737
He et al.	2021	98.959	8.771	0.48	0.03	-1.38	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	273*	–	–
Cavallo et al.	2024	1.96	1.16	–	35	-0.180	–	–	–
Hunt & Reffert	2023	1.90	0.95	0.76	52	–	–	–	–
He et al.	2021	1.82	1.32	–	19	0.169	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 13796	52.0	98.97	8.75	0.48	-0.07	-1.33	–	0.1

💡 Note: The % column shows the percentage of members that HXHWL 58 shares with each listed object.

Visualization

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